在主要组石母体中存在动力机的证据
John A Tarduno1, Rory D Cottrell, Francis Nimmo
1Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA. john.tarduno@rochester.edu
概括
当撞击器核心将液态金属注入原行星时,Pallasite石形成.
科学领域:
- 行星科学 行星科学
- 太空化学 太空化学
- 地质物理学 地质物理学
背景情况:
- 帕拉石是由橄晶和铁金属组成的石铁石.
- 它们的形成起源在石研究中一直是一个长期存在的.
研究的目的:
- 为了调查石石的起源.
- 了解它们形成的条件和过程.
主要方法:
- 在石橄中微小的磁性内含的分析.
- 测量古时强度以确定磁场强度.
- 原行星天体的热建模.
主要成果:
- 帕拉西特橄石含有具有优良记录性能的磁性含有.
- 古磁数据显示了强大的磁场,表明了动力发电机的作用.
- 形成模型表明液体金属注入到原行星的地幔.
结论:
- 帕拉石很可能是从撞击器的核中注入液态铁到原行星的浅地幔时形成的.
- 原行星在撞击后的数百万年里保持完整,允许石的形成.
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