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Growth and Sedimentation of Dust Grains in the Primordial Solar Nebula

Published online by Cambridge University Press:  14 August 2015

Yoshitsugu Nakagawa ,
Kiyoshi Nakazawa  and
Chushiro Hayashi
Yoshitsugu Nakagawa
Affiliation:
Department of Physics, Kyoto University, 606 Japan
Kiyoshi Nakazawa
Affiliation:
Department of Physics, Kyoto University, 606 Japan
Chushiro Hayashi
Affiliation:
Department of Physics, Kyoto University, 606 Japan

Extract

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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
Information
Symposium - International Astronomical Union , Volume 93: Fundamental Problems in the Theory of Stellar Evolution , 1981 , pp. 131 - 132
Copyright
Copyright © Reidel 1981