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月球上的20亿年历史的火山活动
Qiu-Li Li1, Qin Zhou2, Yu Liu1
1State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
Nature
|October 19, 2021
概括
最年轻的月球玄武岩年龄为203亿年,由5号任务,扩展火山活动. 这种精确的放射测年计算了火山口数量,并揭示了月球基岩的KREEP-贫乏地幔来源.
科学领域:
- 月球地质和地化学
- 星球科学
- 放射测年法
背景情况:
- 月球的岩和热量历史不同于陆地行星.
- 大多数月球基岩岩都在28亿年前消失.
- 以前对较年轻的玄武岩的年龄估计依赖于不确定的火山口计数时间表.
研究的目的:
- 为了准确地追溯石团返回的时间.
- 确定这些年轻的月球基岩的分化和来源特征.
- 延长已知月球火山活动的持续时间和时间表.
主要方法:
- 基岩石的- (Pb-Pb) 放射测年.
- 确定包括μ值在内的- (U-Pb) 同位素比率.
- 同位素数据与现有的月球玄武岩数据集的比较.
主要成果:
- 精确的结晶年龄为2,030±400万年前的石.
- 这代表了月球基岩的最年轻的放射年龄,延长了8亿到9亿年的火山活动.
- 基岩来源的μ值很低 (大约 680),表示KREEP缺乏成分.
结论:
- 月球上的火山活动比以前通过放射测年法确定的时间晚得多.
- 精确的年龄为太阳系内部的火山口计时提供了关键的校准点.
- 这些发现为月球的火山和热演变提供了新的见解,突出了这些晚期玄武岩的KREEP-贫穷来源.
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