Coagulation of grains in the solar nebula should result in formation of low-density aggregates with fractal structure. The opacity of the nebula remains much higher than computed for the assumption that particles are compact. Timescales for particle growth, settling to the central plane of the nebula, and formation of planetesimals are lengthened significantly.
Early stages of accumulation in the solar nebula
Advances in Space Research ; 10 , 4-Mar
1990-01-01
Miscellaneous
No indication
English
Early stages of accumulation in the solar nebula
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