从月球背面收集的玄武岩来源的同位素和组成限制
Xiaochao Che1,2, Tao Long1,2, Alexander Nemchin1,3
1Beijing Sensitive High Resolution Ion Micro Probe Center, Institute of Geology, Chinese Academy of Geological Sciences, Beijing, China.
概括
6号任务分析了南极-艾特肯盆地的月球玄武岩. 这些玄武岩表明月球岩海洋 (LMO) 的晚期结晶和SPA冲击的潜在地幔修饰.
科学领域:
- 月球地质和火山活动
- 星球科学
- 地质时间学
背景情况:
- 月球上的火山活动造成了基本岩石沉积,
- 6号任务成功地从月球远端的南极-艾特肯盆地 (SPA) 提取了样本.
研究的目的:
- 分析岩碎片的组成和年龄.
- 研究这些玄武岩对月球内部过程和月球岩海洋 (LMO) 模型的影响.
主要方法:
- 分析岩碎片由6任务收集.
- - (U-Pb) 测定时间,以确定玄武岩的年龄和来源特征.
主要成果:
- 6基岩的构成与低的阿波罗基岩相似.
- 根据U-Pb的测定,基岩年龄为2823.0±590万年.
- 高源238U/204Pb比 (μ值) 为480±56表明LMO结晶的晚期阶段.
结论:
- 这些发现支持月球岩海洋 (LMO) 模型,但显示出与阿波罗样本趋势的偏差.
- 6的基岩数据表明,地幔在LMO后发生了变化,可能与SPA影响有关.
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