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Growth and Sedimentation of Dust Grains in the Primordial Solar Nebula
Published online by Cambridge University Press: 14 August 2015
Extract
Of the formation processes of the solar system, the process of growth and sedimentation of dust particles in the primordial solar nebula is investigated for a region near the Earth's orbit. The growth equation for dust particles, which are sinking as well as in thermal motion, is solved numerically in the wide mass range between 10−12 g and 106 g.
- Type
- Session 3: Origin of the Solar System
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- Copyright
- Copyright © Reidel 1981