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
โฆ LIBER โฆ
Did rotation of the protoplanets originate from the successive collisions of planetesimals?
โ Scribed by Shigeru Ida; Kiyoshi Nakazawa
- Publisher
- Elsevier Science
- Year
- 1990
- Tongue
- English
- Weight
- 805 KB
- Volume
- 86
- Category
- Article
- ISSN
- 0019-1035
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