In a viscously expanding disk, the relative locations of the reaction line and the stagnation line determine whether chemically processed dust is retained or exported; this can explain cometary crystalline silicates with a compact, moderately massive, weakly turbulent protosolar disk.
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Distribution of Chemically-Processed Dust in a Viscously Evolving Protoplanetary Disk: Application to Crystalline Silicates in Comets
In a viscously expanding disk, the relative locations of the reaction line and the stagnation line determine whether chemically processed dust is retained or exported; this can explain cometary crystalline silicates with a compact, moderately massive, weakly turbulent protosolar disk.