Showing 41 - 60 results of 485 for search '"meteorites"', query time: 0.07s Refine Results
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    Silicon isotopes in meteorites and planetary core formation by Armytage, R, Georg, R, Savage, P, Williams, H, Halliday, A

    Published 2011
    “…No systematic δ30Si differences are resolved between chondrites (δ30Si=-0.49±0.15‰, 2σSD) and achondrites (δ30Si=-0.47±0.11‰, 2σSD), although enstatite chondrites are consistently lighter (δ30Si=-0.63±0.07‰, 2σSD) in comparison to other meteorite groups. The data reported here for meteorites and terrestrial samples display an average difference Δ30SiBSE-meteorite*=0.15±0.10‰, which is consistent within uncertainty with previous studies. …”
    Journal article
  3. 43

    Variations in the magnetic properties of meteoritic cloudy zone by Nichols, CIO, Bryson, JFJ, Blukis, R, Herrero-Albillos, J, Kronast, F, Rueffer, R, Chumakov, AI, Harrison, RJ

    Published 2020
    “…Iron and stony‐iron meteorites form the Widmanstätten pattern during slow cooling. …”
    Journal article
  4. 44

    Oxidized conditions in iron meteorite parent bodies by Bonnand, P, Halliday, A

    Published 2018
    “…Magmatic iron meteorites are thought to originate from the cores of differentiated planetary embryos, but it is unclear where they formed in the circumstellar disk. …”
    Journal article
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    Find a falling star/ by 207819 Nivinger, Harvey H.

    Published 1972
    Subjects: “…Meteorites…”
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    Formation of nickel–iron meteorites by chemical fluid transport by Werner Schrön

    Published 2016-09-01
    “…The presence of meteorite alteration and the observed deviations from the solar elemental abundances in silicate meteorites are also explained in terms of the effectiveness of CFT-based mobilization. …”
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    Article
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    Formation of nickel–iron meteorites by chemical fluid transport by Werner Schrön

    Published 2019-01-01
    “…The presence of meteorite alteration and the observed deviations from the solar elemental abundances in silicate meteorites are also explained in terms of the effectiveness of CFT-based mobilization.…”
    Get full text
    Article
  14. 54

    Formation of nickel–iron meteorites by chemical fluid transport by Werner Schrön

    Published 2017-09-01
    “…The presence of meteorite alteration and the observed deviations from the solar elemental abundances in silicate meteorites are also explained in terms of the effectiveness of CFT-based mobilization.…”
    Get full text
    Article
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    Probing the use of spectroscopy to determine the meteoritic analogues of meteors by Drouard, A, Vernazza, P, Loehle, S, Gattacceca, J, Vaubaillon, J, Zanda, B, Birlan, M, Bouley, S, Colas, F, Eberhart, M, Hermann, T, Jorda, L, Marmo, C, Meindl, A, Oefele, R, Zamkotsian, F, Zander, F

    Published 2018
    “…<p><strong>Context:</strong><br /> Determining the source regions of meteorites is one of the major goals of current research in planetary science. …”
    Journal article
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    Meteorite evidence for partial differentiation and protracted accretion of planetesimals by Bryson, J, Maurel, C, Lyons, R, Ball, M, Chopdekar, R, Scholl, A, Ciesla, F, Bottke, W, Weiss, B

    Published 2020
    “…Modern meteorite classification schemes assume that no single planetary body could be source of both unmelted (chondritic) and melted (achondritic) meteorites. …”
    Journal article
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    Laser Raman Induced Degradation of Macromolecular Carbon in Coals and Meteorites by Ryan S. Jakubek, Marc D. Fries

    Published 2023-06-01
    “…MMC is found in geologic samples, such as coals, meteorites, and metamorphic rocks, and the microstructure of the MMC provides details of the thermal history of the sample. …”
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    Article