在一个金属小行星中产生可测量的磁场,其核心是废墟堆
Zhongtian Zhang1, David Bercovici1
1Department of Earth and Planetary Sciences, Yale University, New Haven, CT 06511.
概括
在IVA群铁石的磁场.
科学领域:
- 行星科学 行星科学
- 地质物理学 地质物理学
- 太空化学 太空化学
背景情况:
- 来自IVA群铁石的古磁记录表明它们的母小行星有一个内部磁场.
- 金属小行星的内向固化通常会由于轻元素释放而抑制发电机活动.
- 在这样的天体中磁性的起源仍然是一个.
研究的目的:
- 提出一种新的情景,解释一个向内固化的金属小行星中磁场的产生.
- 解决内部固化和动力发电机活动之间的悖论.
主要方法:
- 小行星形成和热演变的理论建模.
- 假设一个涉及预冷金属碎片的再生现场.
- 研究热提取机制及其对核心动态的影响.
主要成果:
- 提出了一个场景,一个由预冷碎片形成的冷,废墟堆内核从液体金属外核中提取热量.
- 这种热提取驱动固化和轻元素在内核边界的驱逐,为动力发电机提供动力.
- 磁场记录发生在向内增长的地中,因为它冷却低于残留获取温度.
结论:
- 拟议的模型为IVA群石中记录的磁场提供了一个合理的解释.
- 小行星碰撞和再造过程可以创造独特的条件来产生内部动力.
- 这项研究揭示了行星体的早期磁史.
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