太阳星云的寿命受石古磁场的限制
Huapei Wang1, Benjamin P Weiss2, Xue-Ning Bai3
1Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA. huapei@mit.edu.
概括
火山岩分析显示,太阳星云在4.5635亿年前分散,限制了行星形成的时间线,并支持了后来的状星团形成. 这表明太阳系的早期进化发生得很快.
科学领域:
- 星球科学
- 地质学
- 宇宙化学
背景情况:
- 行星的形成涉及气态和磁性太阳星云的演变.
- 太阳星云及其磁场的确切寿命仍然有限,影响我们对早期太阳系过程的理解.
研究的目的:
- 使用古磁分析确定太阳星云分散的时间.
- 确定气态巨星的形成时间和行星迁移的限制.
- 调查圆柱体的形成机制和核心动力发动机的启动.
主要方法:
- 对火山石的古磁分析.
- 用放射测年法确定确切的形成年龄
主要成果:
- 石在4563.5 ± 0.1百万年前形成,其磁场接近于零 (<0.6微位数).
- 这个年龄表明太阳星云及其磁场在太阳系形成后大约380万年已经分散.
- 石母体的核心动力发电机是在太阳系形成后的411亿年开始的.
结论:
- 太阳星云的寿命比以前认为的要短,为气体巨星的形成和行星迁移设定了关键的时间尺度.
- 在星云分散后,可能是通过行星小碰撞形成的.
- 愤怒的母体核心动力发动机的晚期启动表明不同的内部进化途径.
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