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Breakup of liquids by high velocity flow and size distribution of chondrules
Authors:Toshihiko Kadono  Masahiko Arakawa
Institution:a Institute for Research on Earth Evolution, Japan Agency for Marine-Earth Science and Technology, Kanagawa 227-0033, Japan
b Department of Complexity Science and Engineering, University of Tokyo Kashiwanoha 5-1-5, Kashiwa, Chiba 277-8561, Japan
c Institute of Low Temperature Science, Hokkaido University, Sapporo 060-0819, Japan
Abstract:As a new approach to understanding the chondrule formation process, we carried out aerodynamic experiments in which a liquid layer was attached to solid cores, and the breakup of this layer occurred by means of the interaction with a high-velocity gas flow. The size distribution of the dispersed droplets was investigated and compared with the size distributions of chondrules. Both distributions had an exponential form. Using the experimental results, the hydrodynamic pressure to produce the chondrule size distributions was estimated to be ∼ 104 Pa.
Keywords:Meteorites  Origin  Solar System  Solar nebula
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