The effects of tidal forces on the stability and dispersal rates of a protoplanet.
The effects of tidal forces on the stability and dispersal rates of a protoplanet.
复制标题
DOI：
10.1093/mnras/172.2.257
复制
发表时间：
1975-08
影响因子：
4.8
通讯作者：
J. R. Donnison;I. Williams
中科院分区：
文献类型：
--
作者：
J. R. Donnison;I. Williams
太阳对原行星的潮汐破坏被认为是通过分析和数值方法。它的结论是，中断过程是非常迅速的，这意味着，最传统的原行星理论的行星形成需要修改，否则完全中断会发生之前，耐火材料的核心可以形成。
The tidal disruption of a protoplanet by the Sun is considered by both analytical and numerical means. It is concluded that the disruption process is very rapid and that this implies that most conventional protoplanetary theories for the formation of planets need to be modified otherwise complete disruption would have occurred before a refractory core could form.