埃里斯的内部结构是从它的旋转和轨道演变中推断出来的
Francis Nimmo1, Michael E Brown2
1Department of Earth and Planetary Sciences, University of California Santa Cruz, Santa Cruz CA 95064, USA.
Science advances
|November 15, 2023
概括
矮行星埃里斯需要冰冷的外和对流的内部来解释其与迪斯诺米亚的潮锁定. 这种内部活动对于在太阳系年龄的过程中散发能量至关重要.
科学领域:
- 行星科学 行星科学
- 天文学 天文学
- 柯伊伯带的物体 柯伊伯带的物体
背景情况:
- 矮行星Eris与它的卫星Dysnomia被潮锁定.
- 最近对迪斯诺米亚的质量估计表明,埃里斯出乎意料地消散.
研究的目的:
- 为了解释观测到的Eris的潮锁定和消散.
- 确定Eris的内部结构和流程.
主要方法:
- 对Eris-Dysnomia系统动态的分析.
- 模拟埃里斯的内部热演变和结构.
主要成果:
- 埃里斯一定已经分化为冰和岩石核心.
- 埃里斯的冰必须是对流的,以 account 足够的消散.
- 这与冥王星可能的导电冰形成了鲜明对比.
结论:
- 对流动的冰对于像爱丽丝这样的高度散射的天体是必要的.
- 埃里斯的挥发性耗尽可能解释它的对流,不像冥王星.
- 撞击历史可能是Eris独特特征的原因.
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