概括
碳状石中的磁石可能是在它们的母体上形成的,而不是在早期的太阳星云中. 这一发现重新确定了石的日期.
科学领域:
- 宇宙化学 宇宙化学
- 行星科学 行星科学
- 矿物学是一门学科.
背景情况:
- 在CI碳状石中的磁铁石表现出与原始太阳星云中形成不一致的特征.
- 其他形成场景,如石母体上的二次矿化,需要进行调查.
研究的目的:
- 为了确定在CI碳状石中发现的磁铁的起源.
- 重新评估基于磁铁形成的石约会的时间意义.
主要方法:
- 在CI碳状石中分析磁铁的组成和形态.
- 对分析的磁石样本的- (I-Xe) 年代测定.
主要成果:
- 观察到的磁铁的组成和形态强烈地表明了二次起源.
- 石母体上的形成是一个比星云凝结更合理的解释.
结论:
- 这种磁石的-年龄可以追溯到小行星上的二次矿化.
- 这个年龄并不代表太阳星云中的初级凝聚时代.
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