由于巨大的撞击,木星稀释的核心形成
Shang-Fei Liu1,2, Yasunori Hori3,4, Simon Müller5
1School of Physics and Astronomy, Sun Yat-sen University, Zhuhai, China. liushangfei@mail.sysu.edu.cn.
Nature
|August 16, 2019
概括
由于木星的稀释核心, 挑战了行星形成理论. 巨大的撞击可以解释这种结构的核心和混合元素, 符合数十亿年的进化.
科学领域:
- 星球科学
- 天体物理学
- 星球的形成和进化
背景情况:
- 朱诺号的任务揭示了木星的引力场,
- 标准的行星形成模型预测了早期形成的紧核心,在气体捕获过程中积累最小,这与木星观察到的结构相矛盾.
研究的目的:
- 调查解释木星稀释核心和重元素分布的机制,挑战现有的行星形成理论.
- 模拟巨大碰撞对气体巨星内部结构的影响.
主要方法:
- 分析木星重力场上的朱诺任务数据.
- 开发和模拟行星形成模型,包括巨型撞击场景.
- 模拟核心侵蚀和对流混合过程.
主要成果:
- 模型显示行星胚胎和原木星之间的巨大撞击可能会破坏一个紧的核心,
- 这种巨大的撞击场景与木星的内部结构和重元素分布一致.
结论:
- 巨大的撞击是形成像木星这样的稀释核心的可信机制.
- 这种碰撞可能在太阳系早期很常见,并且可以解释木星和土星之间的结构差异.
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