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Chapter 10. Growth of Dust Grains in the Turbulent Solar Nebula

✍ Scribed by Mizuno, Hiroshi


Book ID
118166444
Publisher
Oxford University Press
Year
1988
Tongue
English
Weight
1014 KB
Volume
96
Category
Article
ISSN
0375-9687

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Anticipating the results from the Rosetta magnetometer experiment, we present a theoretical study concerning the possible origin of a cometary magnetic field. Assuming the existence of a permanently magnetized iron dust fraction in the primordial solar nebula, we use a numerical model to investigate