... consider astandard model of the early solar gas disk (Iida et al., 2001).1.2 Physical properties of chondrulesThe chondrule formation models, including the shock-wave heating model, are required ... perturbaritz, SAND2001 -144 0, Sandia National Laboratories, 2001 [32] Sun Chengwei, One dimensional shock and detonation wave computation code SSS, Computation Physics, No.3, 1986: 143 -145 [33] Burgess ... themost serious unsolved problems in planetary science.The most plausible model for chondrule formation is a shock-wave heating model, whichhas been tested by many theoreticians (Ciesla & Hood,...