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    Demonstration of crystalline forsterite grain formation due to coalescence growth of Mg and SiO smoke particles

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    Author
    Kaito, C.
    Ojima, Y.
    Kamitsuji, K.
    Kido, O.
    Kimura, Y.
    Suzuki, H.
    Sato, T.
    Nakada, T.
    Saito, Y.
    Koike, C.
    Issue Date
    2003-01-01
    Keywords
    forsterite
    grain formation
    
    Metadata
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    Citation
    Kaito, C., Ojima, Y., Kamitsuji, K., Kido, O., Kimura, Y., Suzuki, H., ... & Koike, C. (2003). Demonstration of crystalline forsterite grain formation due to coalescence growth of Mg and SiO smoke particles. Meteoritics & Planetary Science, 38(1), 49-57.
    Publisher
    The Meteoritical Society
    Journal
    Meteoritics & Planetary Science
    URI
    http://hdl.handle.net/10150/655642
    DOI
    10.1111/j.1945-5100.2003.tb01045.x
    Additional Links
    https://meteoritical.org/
    Abstract
    Experimental studies of coalescence between Mg grains and SiO grains in smoke reveal the direct production of crystalline forsterite grains. The present results also show that different materials can be produced by grain­grain collisions, which have been considered one of the models of grain formation in the interstellar medium. The fundamentals of coalescence growth in smoke, which have been developed in our series of experiments, are presented in this paper. Mg2Si polyhedral grains were obtained in a Mg grain-rich atmosphere. Mg2SiO4 polyhedral grains were obtained in a SiO grain-rich atmosphere. The IR spectra of the resultant grains showed the characteristics of crystalline forsterite.
    Type
    Article
    text
    Language
    en
    ISSN
    1945-5100
    ae974a485f413a2113503eed53cd6c53
    10.1111/j.1945-5100.2003.tb01045.x
    Scopus Count
    Collections
    Meteoritics & Planetary Science, Volume 38, Number 1 (2003)

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