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Updated: Jun 24, 2026

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Investigation of Early Plasma Evolution Induced by Ultrashort Laser Pulses
Published on: July 2, 2012
太阳系内部的早期进化:一个流星的视角
C M O'D Alexander1, A P Boss, R W Carlson
1Department of Terrestrial Magnetism, Carnegie Institution of Washington, 5241 Broad Branch Road, N.W., Washington, DC 20015, USA.
概括
太阳系中的太阳系.
科学领域:
- 行星科学 行星科学
- 天体物理学 天体物理学
- 宇宙化学 宇宙化学
背景情况:
- 太阳系形成理论 太阳系形成理论
- 太阳系早期的进化过程
- 石的组成和起源
研究的目的:
- 研究太阳系固体的起源.
- 确定石的形成机制.
- 重建早期太阳系过程的时间表.
主要方法:
- 对石组成的分析.
- 太阳系材料的放射测年法
- 原行星盘进化的建模.
主要成果:
- 石中短寿命的放射性核素表明有能粒子辐射的辐射.
- 富含和的含和孔德鲁可能在小行星带中形成.
- 在T Tauri磁盘中形成的体石,可能保留了更高温度的记忆.
结论:
- 地球上的水很可能起源于木星附近的携带水的小行星或冰冷的小行星.
- 地球行星的形成发生在太阳星云分散后.
- 太阳系的进化涉及到磁盘的形成,双极喷气和随后的分化.
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