We have performed N-body simulation on final accretion stage of terrestrial planets, including the effect of damping of eccentricity and inclination caused by tidal interaction with a remnant gas disk. As a result of runway and oligarchic accretion, about 20 Marssized protoplanets would be formed in
โฆ LIBER โฆ
Formation of terrestrial planets in a dissipating gas disk with Jupiter and Saturn
โ Scribed by Junko Kominami; Shigeru Ida
- Book ID
- 108138512
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 430 KB
- Volume
- 167
- Category
- Article
- ISSN
- 0019-1035
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