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  • 1
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    American Association for the Advancement of Science (AAAS)
    Publikationsdatum: 2000-01-05
    Beschreibung: Nitrogen and argon isotopes were measured in carbonatites and associated rocks from the Kola Peninsula in Russia. The Kola mantle source, which is thought to be located in the deep mantle, is enriched in heavy nitrogen (+3 per mil relative to air) as compared to Earth's surface (atmosphere and crust, +2 per mil) and the shallow mantle (-4 per mil). Recycling of oceanic crust (+6 per mil) or metal-silicate partitioning may account for the nitrogen isotopic composition of the deep mantle.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Dauphas -- Marty -- New York, N.Y. -- Science. 1999 Dec 24;286(5449):2488-90.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Centre de Recherches Petrographiques et Geochimiques, CNRS UPR 9046, 15 rue Notre-Dame des Pauvres, Boite Postale 20, 54501 Vandoeuvre-les-Nancy Cedex, France. Ecole Nationale Superieure de Geologie, rue du doyen Marcel Roubault, Boit.〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/10617459" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
    Standort Signatur Erwartet Verfügbarkeit
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  • 2
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    Unbekannt
    American Association for the Advancement of Science (AAAS)
    Publikationsdatum: 2000-11-10
    Beschreibung: Ion microprobe analyses show that solar wind nitrogen associated with solar wind hydrogen implanted in the first tens of nanometers of lunar regolith grains is depleted in 15N by at least 24% relative to terrestrial atmosphere, whereas a nonsolar component associated with deuterium-rich hydrogen, detected in silicon-bearing coatings at the surface of some ilmenite grains, is enriched in 15N. Systematic enrichment of 15N in terrestrial planets and bulk meteorites relative to the protosolar gas cannot be explained by isotopic fractionation in nebular or planetary environments but requires the contribution of 15N-rich compounds to the total nitrogen in planetary materials. Most of these compounds are possibly of an interstellar origin and never equilibrated with the 15N-depleted protosolar nebula.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Hashizume, K -- Chaussidon, M -- Marty, B -- Robert, F -- New York, N.Y. -- Science. 2000 Nov 10;290(5494):1142-5.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Centre de Recherches Petrographiques et Geochimiques-CNRS, BP 20, 54501 Vandoeuvre-les-Nancy Cedex, France. kohash@ess.sci.osaka-u.ac.jp〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/11073449" target="_blank"〉PubMed〈/a〉
    Schlagwort(e): Argon ; Deuterium ; Extraterrestrial Environment ; Hydrogen ; Isotopes ; *Moon ; *Nitrogen ; Nitrogen Isotopes ; Solar System
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
    Standort Signatur Erwartet Verfügbarkeit
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  • 3
    Publikationsdatum: 2004-12-18
    Beschreibung: Archean rocks may provide a record of early Earth environments. However, such rocks have often been metamorphosed by high pressure and temperature, which can overprint the signatures of their original formation. Here, we show that the early Archean banded rocks from Isua, Akilia, and Innersuartuut, Greenland, are enriched in heavy iron isotopes by 0.1 to 0.5 per mil per atomic mass unit relative to igneous rocks worldwide. The observed enrichments are compatible with the transport, oxidation, and subsequent precipitation of ferrous iron emanating from hydrothermal vents and thus suggest that the original rocks were banded iron formations (BIFs). These variations therefore support a sedimentary origin for the Akilia banded rocks, which represent one of the oldest known occurrences of water-laid deposits on Earth.〈br /〉〈span class="detail_caption"〉Notes: 〈/span〉Dauphas, Nicolas -- van Zuilen, Mark -- Wadhwa, Meenakshi -- Davis, Andrew M -- Marty, Bernard -- Janney, Philip E -- New York, N.Y. -- Science. 2004 Dec 17;306(5704):2077-80.〈br /〉〈span class="detail_caption"〉Author address: 〈/span〉Origins Laboratory, Department of the Geophysical Sciences, and Enrico Fermi Institute, University of Chicago, 5734 South Ellis Avenue, Chicago, IL 60637, USA. dauphas@uchicago.edu〈br /〉〈span class="detail_caption"〉Record origin:〈/span〉 〈a href="http://www.ncbi.nlm.nih.gov/pubmed/15604404" target="_blank"〉PubMed〈/a〉
    Print ISSN: 0036-8075
    Digitale ISSN: 1095-9203
    Thema: Biologie , Chemie und Pharmazie , Informatik , Medizin , Allgemeine Naturwissenschaft , Physik
    Standort Signatur Erwartet Verfügbarkeit
    BibTip Andere fanden auch interessant ...
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