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The Stability of Protoplanet Systems

โœ Scribed by Keiko Yoshinaga; Eiichiro Kokubo; Junichiro Makino


Publisher
Elsevier Science
Year
1999
Tongue
English
Weight
317 KB
Volume
139
Category
Article
ISSN
0019-1035

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Planetary accretion from planetesimals to protoplanets is investigated using three-dimensional N-body simulations. The effect of gas drag due to solar nebula is included and realistic-sized planetesimals with a standard material density are used, with which the growth time scale of planetesimals is