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  <rdf:Description rdf:about="https://doi.org/10.1016/j.epsl.2016.12.008">
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    <dct:isPartOf>Earth and Planetary Science Letters</dct:isPartOf>
    <dct:license>Open Access</dct:license>
    <dct:created>2016-12-22</dct:created>
    <dct:available>2016-01-01</dct:available>
    <dct:available>2020-08-20</dct:available>
    <dc:description>Non-mass dependent chromium isotopic signatures have been successfully used to determine the presence and identification of extra-terrestrial materials in terrestrial impact rocks. Paleoproterozoic spherule layers from Greenland (Graenseso) and Russia (Zaonega), as well as some distal ejecta deposits (Lake Superior region) from the Sudbury impact (1,849 +/- 0.3 Ma) event, have been analyzed for their Cr isotope compositions. Our results suggest that 1) these distal ejecta deposits are all of impact origin, 2) the Graenseso and Zaonega spherule layers contain a distinct carbonaceous chondrite component, and are possibly related to the same impact event, which could be Vredefort (2,023 +/- 4 Ma) or another not yet identified large impact event from that of similar age, and 3) the Sudbury ejecta record a complex meteoritic signature, which is different from the Graenseso and Zaonega spherule layers, and could indicate the impact of a heterogeneous chondritic body.</dc:description>
    <dc:subject>TERRESTRIAL</dc:subject>
    <dc:subject>KARELIA</dc:subject>
    <dc:subject>impact ejecta</dc:subject>
    <dc:subject>FOS: Physical sciences</dc:subject>
    <dc:subject>01 natural sciences</dc:subject>
    <dc:subject>METEORITIC COMPONENTS</dc:subject>
    <dc:subject>SOLAR-SYSTEM</dc:subject>
    <dc:subject>[SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology</dc:subject>
    <dc:subject>[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/Geochemistry</dc:subject>
    <dc:subject>SOUTH GREENLAND</dc:subject>
    <dc:subject>[SDU.STU.GC] Sciences of the Universe [physics]/Earth Sciences/Geochemistry</dc:subject>
    <dc:subject>GEOCHEMICAL EVIDENCE</dc:subject>
    <dc:subject>Vredefort</dc:subject>
    <dc:subject>Sudbury</dc:subject>
    <dc:subject>0105 earth and related environmental sciences</dc:subject>
    <dc:subject>Earth and Planetary Astrophysics (astro-ph.EP)</dc:subject>
    <dc:subject>crater</dc:subject>
    <dc:subject>KETILIDIAN OROGEN</dc:subject>
    <dc:subject>meteorite</dc:subject>
    <dc:subject>EARLY EARTH</dc:subject>
    <dc:subject>105105 Geochemistry</dc:subject>
    <dc:subject>EVENT</dc:subject>
    <dc:subject>13. Climate action</dc:subject>
    <dc:subject>chromium isotopes</dc:subject>
    <dc:subject>[SDU.STU.PL] Sciences of the Universe [physics]/Earth Sciences/Planetology</dc:subject>
    <dc:subject>105105 Geochemie</dc:subject>
    <dc:subject>SPHERULES</dc:subject>
    <dc:subject>Astrophysics - Earth and Planetary Astrophysics</dc:subject>
    <dc:creator rdf:resource="https://orcid.org/0000-0001-5155-7405"/>
    <dc:creator>Christian Koeberl, Christian Koeberl, Christa G&#246;pel, B&#233;reng&#232;re Mougel, Fr&#233;d&#233;ric Moynier, Fr&#233;d&#233;ric Moynier, </dc:creator>
    <dc:date>2017-02-01</dc:date>
    <dc:type>journalpaper</dc:type>
    <dct:abstract>Non-mass dependent chromium isotopic signatures have been successfully used to determine the presence and identification of extra-terrestrial materials in terrestrial impact rocks. Paleoproterozoic spherule layers from Greenland (Graenseso) and Russia (Zaonega), as well as some distal ejecta deposits (Lake Superior region) from the Sudbury impact (1,849 +/- 0.3 Ma) event, have been analyzed for their Cr isotope compositions. Our results suggest that 1) these distal ejecta deposits are all of impact origin, 2) the Graenseso and Zaonega spherule layers contain a distinct carbonaceous chondrite component, and are possibly related to the same impact event, which could be Vredefort (2,023 +/- 4 Ma) or another not yet identified large impact event from that of similar age, and 3) the Sudbury ejecta record a complex meteoritic signature, which is different from the Graenseso and Zaonega spherule layers, and could indicate the impact of a heterogeneous chondritic body.</dct:abstract>
    <dc:title>Chromium isotope evidence in ejecta deposits for the nature of Paleoproterozoic impactors</dc:title>
    <dc:identifier>10.1016/j.epsl.2016.12.008</dc:identifier>
    <dct:references>https://doi.org/10.1016/j.epsl.2016.12.008</dct:references>
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