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  • 11
    Publication Date: 2024-01-09
    Keywords: 183-1137A; Anorthite; Barium; Barium, partition coefficient; Cerium; Cerium, partition coefficient; DRILL; Drilling/drill rig; DSDP/ODP/IODP sample designation; Indian Ocean; Joides Resolution; Lanthanum; Lanthanum, partition coefficient; Leg183; Neodymium; Neodymium, partition coefficient; Ocean Drilling Program; ODP; Praseodymium; Praseodymium, partition coefficient; Rubidium; Rubidium, partition coefficient; Samarium; Samarium, partition coefficient; Sample code/label; Sample code/label 2; Sample comment; Strontium; Strontium, partition coefficient; Yttrium; Yttrium, partition coefficient
    Type: Dataset
    Format: text/tab-separated-values, 660 data points
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  • 12
    Publication Date: 2024-01-09
    Keywords: 183-1137A; Aluminium oxide; Anorthite; Barium; Calcium oxide; Cerium; DRILL; Drilling/drill rig; DSDP/ODP/IODP sample designation; Electron microprobe (EMP); Elements, total; Europium; Indian Ocean; Iron oxide, FeO; Joides Resolution; LA-ICP-MS, Laser-ablation inductively coupled plasma mass spectrometer; Lanthanum; Lead; Leg183; Magnesium oxide; Neodymium; Ocean Drilling Program; ODP; Phosphorus pentoxide; Potassium oxide; Praseodymium; Rubidium; Samarium; Sample code/label; Sample code/label 2; Sample comment; Scandium; Silicon dioxide; Sodium oxide; Strontium; Titanium; Titanium dioxide; Vanadium; Yttrium
    Type: Dataset
    Format: text/tab-separated-values, 756 data points
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  • 13
    Publication Date: 2024-01-09
    Keywords: 183-1137A; Anorthite; Barium; Barium, partition coefficient; Cerium; Cerium, partition coefficient; DRILL; Drilling/drill rig; DSDP/ODP/IODP sample designation; Indian Ocean; Joides Resolution; Lanthanum; Lanthanum, partition coefficient; Leg183; Neodymium; Neodymium, partition coefficient; Ocean Drilling Program; ODP; Praseodymium; Praseodymium, partition coefficient; Rubidium; Rubidium, partition coefficient; Samarium; Samarium, partition coefficient; Sample code/label; Sample code/label 2; Sample comment; Strontium; Strontium, partition coefficient; Yttrium; Yttrium, partition coefficient
    Type: Dataset
    Format: text/tab-separated-values, 594 data points
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  • 14
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    PANGAEA
    In:  Supplement to: Chazey III, William J; Neal, Clive R (2005): Platinum group element constraints on source composition and magma evolution of the Kerguelen Plateau using basalts from ODP Leg 183. Geochimica et Cosmochimica Acta, 69(19), 4685-4701, https://doi.org/10.1016/j.gca.2005.02.006
    Publication Date: 2024-01-09
    Description: Seventeen basalts from Ocean Drilling Program (ODP) Leg 183 to the Kerguelen Plateau (KP) were analyzed for the platinum-group elements (PGEs: Ir, Ru, Rh, Pt, and Pd), and 15 were analyzed for trace elements. Relative concentrations of the PGEs ranged from ~0.1 (Ir, Ru) to ~5 (Pt) times primitive mantle. These relatively high PGE abundances and fractionated patterns are not accounted for by the presence of sulfide minerals; there are only trace sulfides present in thin-section. Sulfur saturation models applied to the KP basalts suggest that the parental magmas may have never reached sulfide saturation, despite large degrees of partial melting (~30%) and fractional crystallization (~45%). First order approximations of the fractionation required to produce the KP basalts from an ~30% partial melt of a spinel peridotite were determined using the PELE program. The model was adapted to better fit the physical and chemical observations from the KP basalts, and requires an initial crystal fractionation stage of at least 30% olivine plus Cr-spinel (49:1), followed by magma replenishment and fractional crystallization (RFC) that included clinopyroxene, plagioclase, and titanomagnetite (15:9:1). The low Pd values ([Pd/Pt]_pm 〈 1.7) for these samples are not predicted by currently available Kd values. These Pd values are lowest in samples with relatively higher degrees of alteration as indicated by petrographic observations. Positive anomalies are a function of the behavior of the PGEs; they can be reproduced by Cr-spinel, and titanomagnetite crystallization, followed by titanomagnetite resorption during the final stages of crystallization. Our modeling shows that it is difficult to reproduce the PGE abundances by either depleted upper or even primitive mantle sources. Crustal contamination, while indicated at certain sites by the isotopic compositions of the basalts, appears to have had a minimal affect on the PGEs. The PGE abundances measured in the Kerguelen Plateau basalts are best modeled by melting a primitive mantle source to which was added up to 1% of outer core material, followed by fractional crystallization of the melt produced. This reproduces both the abundances and patterns of the PGEs in the Kerguelen Plateau basalts. An alternative model for outer core PGE abundances requires only 0.3% of outer core material to be mixed into the primitive mantle source. While our results are clearly model dependent, they indicate that an outer core component may be present in the Kerguelen plume source.
    Keywords: 183-1136A; 183-1137A; 183-1138A; 183-1141A; 183-1142A; DRILL; Drilling/drill rig; Indian Ocean; Joides Resolution; Leg183; Ocean Drilling Program; ODP
    Type: Dataset
    Format: application/zip, 5 datasets
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  • 15
    Publication Date: 2022-05-26
    Description: Author Posting. © Oceanography Society, 2019. This article is posted here by permission of Oceanography Society for personal use, not for redistribution. The definitive version was published in Neal, C.R., M.F. Coffin, and W.W. Sager. Contributions of scientific ocean drilling to understanding the emplacement of submarine large igneous provinces and their effects on the environment. Oceanography 32(1), (2019):176–192, doi:10.5670/oceanog.2019.142.
    Description: The Ontong Java Plateau (OJP), Shatsky Rise (SR), and Kerguelen Plateau/Broken Ridge (KP/BR) represent three large igneous provinces (LIPs) located in oceanic settings. The basement lavas have been investigated through scientific ocean drilling and, in the case of the OJP, fieldwork on the emergent obducted portions of the plateau in the Solomon Islands. Such studies show that these three LIPs have very different characteristics. For example, the KP/BR still has an active hotspot, whereas the OJP and the SR do not. The OJP is remarkable in its compositional monotony across the plateau (the Kwaimbaita geochemical type), with minor compositional variation found at the margins (the Kroenke, Singgalo, and Wairahito types). Shatsky Rise shows more compositional variation and, like the OJP, has a dominant lava type (termed the “normal” type) in the early stages (Tamu Massif), but subsequent eruptions at the Ori and Shirshov massifs comprise isotopically and trace element enriched lavas, likely reflecting a change in mantle source over time. The KP/BR has highly variable basement lava compositions, ranging from lavas slightly enriched above that of normal mid-ocean ridge basalt in the northern portion (close to the South East Indian Ridge) to more enriched varieties to the south and on Broken Ridge, with a continental crust signature present in lavas from the southern and central KP/BR. The OJP and the KP/BR appear to have formed through punctuated magmatic events, whereas the SR was formed by one relatively long, drawn out event. The formation of oceanic LIPs has in many (but not all) cases been synchronous with oceanic anoxic events. This paper focuses on three oceanic plateaus to emphasize the debate surrounding the environmental impact such LIPs may have had, and also highlights the contributions of scientific ocean drilling to our knowledge of oceanic LIP formation and evolution. This new knowledge allows planning for future oceanic LIP drilling.
    Description: Many thanks to the crew and operators of the scientific ocean drilling vessel JOIDES Resolution without whom the understanding of oceanic flood basalts would be severely limited. We also thank the US National Science Foundation for continued support of scientific ocean drilling. We are indebted to Jörg Geldmacher, Paul Wallace, Carlotta Escutia, and Anthony Koppers for reviews of this paper that were insightful and extremely helpful in making it much better than the initial submission.
    Repository Name: Woods Hole Open Access Server
    Type: Article
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  • 16
    ISSN: 1438-1168
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Description / Table of Contents: Zusammenfassung Der Blue Ball Kimberlit, Scott County, Arkansas, enthält zwischen 23 und 36% Phlogopit (modal). Dieser kommt in idiomorphen Kristallen, als Grundmasse, und als Coronas um serpentinisierte Olivinkristalle vor. Verschiedene Arten von Pleochroismus, die man in den Kernen von Kristallen und in der Mehrzahl der Phlogopite in der Grundmasse erkennen kann, lassen sich mit der Mineralehemie korrelieren. Reverser Pleochroismus ist an den Rändern von Kristallen, selten in Grundkörnern der Grundmasse, und in Phlogopiten die Coronas in Olivin bilden, zu beobachten. Diese Erscheinung wird im allgemeinen von einer Zunahme des Gesamt-Eisens (als FeO) und einer Abnahme der Al2 O3-Gehalte begleitet. Analysen jener Phlogopite, die reversen Pleochroismus zeigen, haben hohe Gesamtwerte an Kationen und dies weist auf die Anwesenheit von Fe3+ hin. Wir interpretieren diesen Pleochroismus als eine Funktion des Fe3+ in der Tetraeder-Position, die sich als ΔT = 8 - (Si + Al) ausdrücken läßt. Alle Phlogopite von Blue Ball haben positive Werte für ΔT, aber reverser Pleochroismus tritt nur dort auf, wo ΔT 〉 0.6, was widerum auf eine Zunahme von Fe3+ im residualen Magma hinweist. Phlogopit war praktisch während der gesamten Kristallisation des Kimberlits am Liquidus, und diese Annahme wird auch durch das weite Feld der PhlogopitZusammensetzungen und durch die allgemeine Abahme der Ba-Gehalte in Glimmern mit intermediärem bis reversem Pleochroismus unterstützt. Variationen von MG #, Ti, Ba, Si und Al in den Phlogopiten wurden benutzt, um die Kristallisation von Olivin und Spinellen (Chromit und Titanomagnetit) zu verfolgen. Olivin hat früh kristallisiert und führte zu einer Abnahme von MG# und Si und einer Zunahme von Ti und Al in den Phlogopiten. Auch kleinere Mengen von Chromit kristallisierten zu dieser Zeit, dies war jedoch nicht ausreichend, um den Effekt der Olivin-Fraktionierung auf die Restschmelze aufzuheben. Titanomagnetit-Kristallisation setzte mit aufhörender Olivinfraktionierung ein und führte zu einer Zunahme von Mg und Si und einer Abnahme von Ti und Al. Eine Überprüfung der chemischen Variationen und Vergleich mit ΔT Werten tragen wesentlich zur Kenntnis der Evolution des Blue Ball Kimberlites bei.
    Notes: Summary The Blue Ball kimberlite, Scott County, Arkansas, contains between 23 and 36 modal % phlogopite. Phlogopite is present as phenocrysts, a groundmass phase, and as coronas around serpentinized olivine phenocrysts. Intermediate and reverse pleochroism, seen in phenocryst cores and the majority of groundmass phlogopites, can be correlated with the mineral chemistry. Reverse pleochroism, exhibited by phenocryst rims, rare groundmass grains, and phlogopites forming coronas around olivine, is generally accompanied by an increase in total Fe (as FeO) and a decrease in Al2 O3. Analyses of those phlogopites whoch exhibit reverse pleochroism have high cation totals, indicative of the presence of Fe3+. We suggest that these pleochroic schemes are a function of Fe3+ in the tetrahedral site, which is expressed in terms of ΔT = [8 - (Si + Al)]. All Blue Ball phlogopites have positive values for ΔT, but reverse pleochroism is found only when ΔT 〉 0.6, indicative of increased Fe3+ in the residual magma. It is concluded that phlogopite was on the liquidus throughout practically all of the kimberlite crystallization, because of the wide range in phlogopite compositions and the general decrease in Ba from micas exhibiting intermediate to reverse pleochroism. Variations of MG #, Ti, Ba, Si, and Al within the phlogopites have been used to trace the crystallization of other phases present in the kimberlite, namely olivine and spinel (chromite and titanomagnetite). Olivine was an early crystallizing phase, causing a decrease in MG # and Si, and an increase in Ti and Al in the phlogopites, a reflection of residual magma composition. Minor chromite also crystallized at this time, but was not of sufficient quantity to override the effect of olivine fractionation on the residual magma. Widespread Titano-magnetite crystallization occurred as olivine fractionation ceased, causing an increase in MG # and Si, and a decrease in Ti and Al. By examining these chemical variations with ΔT, the evolution of the Blue Ball kimberlite has been determined.
    Type of Medium: Electronic Resource
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  • 17
    Electronic Resource
    Electronic Resource
    Springer
    Contributions to mineralogy and petrology 113 (1993), S. 280-284 
    ISSN: 1432-0967
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Notes: Abstract Caporuscio and Smyth have presented crystal chemical study on eleven mantle-derived eclogites from the Bellsbank (8) and Roberts Victor (3) kimberlites, South Africa. They combine these results with experimental partition coefficients and geochemical modelling to argue for a high pressure igneous cumulate origin from a MORB-like melt for these eclogites. In particular, they highlight the kyanite-bearing eclogites (grospydites), especially the presence of a “middle rare-earth-element (MREE) enrichment”, which may also be considered in terms of LREE and HREE depletions. Caporuscio and Smyth, as well as Smyth et al., cite this phenomenon as evidence for an origin by igneous accumulation of hyperaluminous clinopyroxene at high pressure. However, this type of REE pattern has also been interpreted as depicting a positive Eu anomaly inherited from a subducted, plagioclase-rich oceanic crustal protolith (Shervais et al., Taylor and Neal, Neal et al.). This manuscript presents an alternative interpretation of the data presented by Caporuscio and Smyth. The results presented here demonstrate that high-pressure igneous accumulation of hyperaluminous pyroxene from a MORB-like liquid, followed by exsolution of major amounts of garnet and kyanite, is unlikely to account for all chemical signatures exhibited by grospydites. Our approach is to undertake quantitative geochemical modelling of these processes using the actual samples and literature values quoted by Caporuscio and Smyth.
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  • 18
    Publication Date: 2007-10-08
    Description: A total of 16 Ontong Java Plateau (OJP) basalt samples from Ocean Drilling Program Legs 192 and 130 were analysed for major, trace and platinum-group elements (PGEs; Ir, Ru, Rh, Pt and Pd). Major- and trace-element compositions determined by our study confirm Leg 192 shipboard analyses that indicated a new group of more primitive or Kroenke-type' basalts, with higher MgO, Ni and Cr, and lower incompatible-element, abundances than the more common Kwaimbaita-type basalts. The PGE abundances quantified here extend the range of the continuum of compositions found in previously analysed OJP basalts and are similar to those present in some komatiites. The PGEs, therefore, cannot be used to differentiate definitively between OJP basalts groups. The two samples analysed from Leg 130 (one from Site 803 and one from Site 807) are akin to the Kwaimbaita-type basalts. Low-temperature alteration has not affected Pd abundances in the Leg 192 basalts as it has in the Solomon Island and the Leg 130 samples. Elemental abundances and ratios along with petrography reveal that the OJP basalts have not experienced sulphide saturation. Positive correlations of Ir and Ru with Cr and Ni attest to the lithophile behaviour of the PGEs and lend more credence to studies suggesting compatibility of these elements in oxide and silicate phases, such as Cr-spinel and olivine. Estimates of sulphur abundance in the mantle, degree of partial melting and pressure of melt initiation were used in conjunction with the model of Mavrogenes & O'Neill to calculate a minimum initial excess temperature of +185-+235{degrees}C (1465-1515{degrees}C at 3.5-4.0 GPa) above ambient mantle for the OJP source. This is in broad agreement with a fossil geotherm preserved in megacrysts and peridotite xenoliths found in pipe-like intrusives of alnoite that outcrop on the island of Malaita, Solomon Islands. Using the PGEs as a guide, the OJP basalts were modelled using a three-source component melt mix: a 10% garnet peridotite melt of primitive mantle composition, which then passed through the garnet-spinel transition and melted a further 20%, a 30% partial melt of fertile upper mantle and 0-1% of outer core material. The core component was included only in the plume source, and the ratio of plume source to upper mantle source was 19: 1. It is evident from this study that the PGE contents of at least some of the OJP basalts are too high to be generated by primitive mantle sources alone. A PGE-enriched component is required and we suggest that this is outer core material. While a sulphide-rich mantle component could also increase the PGE abundances (assuming that the sulphide is exhausted during partial melting), the sulphur-undersaturated nature of these basalts argues against this. Variations in the amount of outer core in the source (from 0 to 1 wt%) and degree of fractional crystallization can account for the entire range in PGE abundances of OJP basalts.
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  • 19
    Publication Date: 2007-10-08
    Description: Tholeiitic basalts have been recovered from drill sites in different locations on the Ontong Java Plateau (OJP) and are remarkably homogeneous across this large igneous province. The most abundant basalt type is represented by the Kwaimbaita Formation on Malaita in the Solomon Islands, where it is capped by the isotopically distinct and slightly more incompatible-element-enriched basalt of the Singgalo Formation. Ocean Drilling Program (ODP) Leg 192 drilled five sites on the OJP, four of which penetrated basement lava successions. All basalt recovered during Leg 192 is chemically and isotopically indistinguishable from Kwaimbaita-type lavas. Site 1184 of ODP Leg 192 is situated on the eastern salient of the OJP, and is unique because the recovered volcaniclastic succession contains the first conclusive evidence for emergence of part of the OJP above sea level. Within this succession are clasts of basaltic material. We report the major element-, trace-element and isotopic compositions of 14 moderately to highly altered basalt clasts. On the basis of incompatible-element concentrations, specifically high field strength elements (HFSE) and rare earth elements (REE), four groups of clasts are defined. Group 1 clasts are similar to basalt from the Kwaimbaita Formation. Group 2 clasts show variable composition, but the heavy rare earth element (HREE) concentrations are similar to those of basalts from the Kwaimbaita Formation. Group 3 clasts have compositions similar to the high-MgO Kroenke-type basalt recovered during ODP Leg 192. Group 4 clasts are more evolved than the Kwaimbaita or Singgalo lavas, and contain deep negative Eu and Sr anomalies on primitive-mantle (PM)-normalized diagrams, as well as high concentrations of Nb, Ta and Th. Group 4 clasts also show a large fractionation of Nb from La and have (Nb/La)PM ratios of approximately 2. Sr-, Nd- and Pb-isotope ratios were measured on five clasts covering all four groups. Although the Sr- and Pb-isotope ratios exhibit some variability, which we attribute to alteration, the Nd-isotope ratios are within the field defined for Kwaimbaita-type lavas. We conclude that most of the compositional variability displayed by these clasts is a result of alteration and that Ta appears to be the most immobile incompatible trace element. All of the clasts were derived from the mantle source that produced the Kwaimbaita-type and Kroenke-type basalts. Our data emphasize the widespread nature of Kwaimbaita-type basalt and show that the source region was active under both the eastern salient and the high plateau of the OJP.
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  • 20
    Publication Date: 2007-10-08
    Description: The compositions of glass clasts in volcaniclastic rocks recovered from drilling at Site 1184 on the eastern salient of the Ontong Java Plateau (OJP) are investigated using microbeam analytical methods for major, minor and trace elements. These data are compared with whole-rock elemental and isotopic data for bulk tuff samples, and with data from basalts on the high plateau of the OJP. Three subunits of Hole 1184A contain blocky glass clasts, thought to represent the juvenile magmatic component of the phreatomagmatic eruptions that generated the volcaniclastic rocks. The glass clasts have unaltered centres, and are all basaltic low-K tholeiites, with flat chondrite-normalized rare earth element (REE) patterns. Their elemental compositions are very similar to the Kwaimbaita-type and Kroenke-type basalts sampled on the high plateau. Each subunit has a distinct glass composition and there is no intermixing of glass compositions between subunits, indicating that each subunit is the result of one eruptive phase, and that the volcaniclastic sequence has not experienced reworking. The relative heterogeneity preserved at Site 1184 contrasts with the uniformity of compositions recovered from individual sites on the high plateau, and suggests that the eastern salient of the OJP had a different type of magma plumbing system. Our data support the hypothesis that the voluminous subaerially erupted volcaniclastic rocks at Site 1184 belong to the same magmatic event as the construction of the main Ontong Java Plateau. Thus, the OJP would have been responsible for volatile fluxes into the atmosphere in addition to chemical fluxes into the oceans, and these factors may have influenced the contemporaneous oceanic anoxic event.
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