地力发电机,太阳风和磁断发生在34亿至34亿年前
John A Tarduno1, Rory D Cottrell, Michael K Watkeys
1Department of Earth and Environmental Sciences, University of Rochester, Rochester, NY 14627, USA. john@earth.rochester.edu
概括
早期的地球地球.
科学领域:
- 地质物理学 地质物理学
- 古磁论是古磁论的一种学说.
- 行星科学 行星科学
背景情况:
- 行星磁场保护大气层免受恒星风侵蚀.
- 早期地球的可居住性表明有一个保护性的磁场,但它的强度是未知的.
- 了解早期磁场强度对于行星可居住性研究至关重要.
研究的目的:
- 为了确定地球磁场在古阿纪时代的强度.
- 评估早期磁场强度对大气保留和进化的影响.
主要方法:
- 从带有磁性入的单酸盐晶体中分析古强度.
- 利用34亿至34亿5千万年前的地力发电机记录.
主要成果:
- 古代强度测量表明,地球早期的磁场强度为当今磁场的50-70%.
- 结合较高的古老时代太阳风压力,磁断对峙距离估计小于或等于5个地球半径.
- 证据表明较低度的极光和增加的极地面积.
结论:
- 早期地球的磁场足够强大来保护大气和水,支持可居住性.
- 磁层的配置可能通过外层加热和挥发性损失影响了大气组成.
- 这些发现为早期行星可居住性所必需的条件提供了关键的见解.
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