| タイトル | Physics of the primitive solar nebula and of giant gaseous protoplanets |
| 著者（英） | Cameron, A. G. W. |
| 著者所属（英） | Harvard-Smithsonian Center for Astrophysics |
| 発行日 | 1978-01-01 |
| 言語 | eng |
| 内容記述 | It has been proposed that the supernova responsible for injecting Al-26 into the early solar system was in fact responsible for triggering the collapse of an interstellar cloud in order to produce a system of stars, one of which would be the solar system. Details concerning the mechanism involved in such a process are discussed. Attention is given to the evolution of the primitive solar nebula, the instabilities in the primitive solar nebula, and the giant gaseous protoplanets. The principal conclusion to be drawn from the material presented is that the primitive solar nebula was a rather chaotic place, highly turbulent, with the multiple formation of giant gaseous protoplanets. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 79A26799 |
| 権利 | Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/428055 |
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