| 释义 |
- 1
The other model, 'fragmentation', suggests that small clumps of a gaseous disk form directly into planets over 10,000 years. 另一个模型——碎化模型则认为大量聚集的气体盘在10000多年间直接形成了气体行星。 - 2
The other model, 'fragmentation', suggests that small clumps of a gaseous disk form directly into planets over 10, 000 years. 另一个模型——碎化模型则认为大量聚集的气体盘在10000多年间直接形成了气体行星。 - 3
At their distances from the star, the rocky planetary core would have taken so long to form that the gaseous disk would have dissipated before the core could attract the gas. 就它们与恒星的距离而言，其石质行星核恐怕需要极其长的成型时间，以至于在星核能够俘获气体前周围的气态盘恐怕就已经消散殆尽了。
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