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  • 1990-1994  (2)
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  • 1
    Publication Date: 2017-09-26
    Description: Three groups of REE patterns are observed for the sandstones and shales of the Middle Ordovician Austin Glen Member of the Normanskill Formation. One sandstone sample is enriched in middle and light rare earth elements. The majority of samples are light rare earth element (LREE) enriched with negative Eu-anomalies and flat heavy rare earth elements (HREEs), whereas a third group appears to have lost LREEs and middle rare earth element (MREEs). Homogeneous neodymium isotopic compositions for all samples at about the time of deposition, ϵNd (470 Ma) = −8.2 ± 1.1(2SD), indicate that the source of the Austin Glen Member was well mixed and that the neodymium had a long-term enriched history. The differences in the shape and abundances of the REE patterns combined with the neodymium isotope characteristics of the samples lead us to the conclusion that samarium and neodymium were fractionated and that the neodymium isotopic system might have been disturbed at about the time of deposition (470 Ma). Most samples appear to have been affected by this process. The two most altered shales lost about half of their neodymium and their ratios are higher than the ratios of average shales. These two shales give clearly erroneous mantle-extraction ages, but the average TDM of the provenance can still be deduced (1700–1800 Ma) from the least disturbed sandstones with normal upper crustal ratios. Accordingly, this study demonstrates that the REEs may be transported and neodymium isotopes may be reequilibrated under certain sedimentary conditions (e.g., diagenesis). However, in spite of evidence for REE redistribution, provenance information (TDM, original REE patterns) may still be inferred.
    Type: Article , PeerReviewed
    Format: text
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  • 2
    Publication Date: 2018-03-28
    Description: Altered volcanic ashes (K-bentonites) in the late Ordovician (Caradocian) Utica shale of New York State are the product of explosive arc volcanism. Most of the 30 K-bentonites examined in this investigation contain fragmental crystals and rock fragments (microliths) up to 600 (xm in diameter that generally are neither detrital contamination from the surrounding black shale nor igneous phenocrysts. The dominant phases are garnet ($two groups; Gr_{15_20} Alm_{45_75} Py_{35_0} Sp_{2-5}; Gr_{2_5} Alm_{55_85} Py_{10-40} Spi$), plagioclase feldspar ($An{80-10}$), alkali feldspar ($Or_{99_0}$), clinopyroxene $(Wo_{50-40} En_{50-30} Fs_{0-30}$), and orthopyroxene ($Wo_{1-2} En_{77_32} Fs{32_66}4$), accompanied by lesser quantities of hornblende, aluminosilicate, quartz, sphene, Fe-Ti oxides, apatite, and zircon. Most of the fragmental crystals appear to be derived from the same source as the metamorphic microliths, which possess minerals with similar compositions. Both crystals and microliths are interpreted as xenocrysts and xenoliths from the ancient continental crust on which the Ordovician arc was constructed. They became entrained in the volcanic plume during explosive eruptions. A Precambrian age acquired on K-feldspars from one K-bentonite using the $^{40}Ar/^{39}Ar$ method shows that these xenocrysts were derived from depths of less than 5-10 km in the microcontinent at the time of late Ordovician volcanism. The occurrence of xenocrysts and xenoliths in these K-bentonites underscores the importance of performing detailed petrology on ash layers prior to the onset of more sophisticated tasks (e.g., isotopic age determinations; regional stratigraphic correlations of K-bentonites based upon chemical compositions).
    Type: Article , PeerReviewed
    Format: text
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