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    Maximal size of chondrules in shock wave heating model: Stripping of liquid surface in a hypersonic rarefied gas flow

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    Author
    Kato, Takaaki
    Nakamoto, Taishi
    Miura, Hitoshi
    Issue Date
    2006-01-01
    Keywords
    shock effect
    shock heating
    chondrule formations
    shock melt
    
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    Citation
    Kato, T., Nakamoto, T., & Miura, H. (2006). Maximal size of chondrules in shock wave heating model: Stripping of liquid surface in a hypersonic rarefied gas flow. Meteoritics & Planetary Science, 41(1), 49-65.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/656089
    DOI
    10.1111/j.1945-5100.2006.tb00192.x
    Additional Links
    https://meteoritical.org/
    Abstract
    We examined partially molten dust particles that have a solid core and a surrounding liquid mantle, and estimated the maximal size of chondrules in a framework of the shock wave heating model for chondrule formation. First, we examined the dynamics of the liquid mantle by analytically solving the hydrodynamics equations for a core-mantle structure via a linear approximation. We obtained the deformation, internal flow, pressure distribution in the liquid mantle, and the force acting on the solid core. Using these results, we estimated conditions in which liquid mantle is stripped off from the solid core. We found that when the particle radius is larger than about 1-2 mm, the stripping is expected to take place before the entire dust particle melts. So chondrules larger than about 1-2 mm are not likely to be formed by the shock wave heating mechanism. Also, we found that the stripping of the liquid mantle is more likely to occur than the fission of totally molten particles. Therefore, the maximal size of chondrules may be determined by the stripping of the liquid mantle from the partially molten dust particles in the shock waves. This maximal size is consistent with the sizes of natural chondrules.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2006.tb00192.x
    Scopus Count
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    Meteoritics & Planetary Science, Volume 41, Number 1 (2006)

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