月球远端地幔衍生物质的Chang'E-4初始光谱识别
Chunlai Li1, Dawei Liu2, Bin Liu2
1Key Laboratory of Lunar and Deep Space Exploration, National Astronomical Observatories, Chinese Academy of Sciences, Beijing, China. licl@nao.cas.cn.
Nature
|May 17, 2019
概括
在中国
科学领域:
- 星球科学
- 月球地质
- 矿物学
背景情况:
- 月球的地主要是层,覆盖着由岩海洋形成的不确定的地.
- 大型冲击盆地,如南极-艾特肯 (SPA) 盆地,可能会暴露地幔物质.
- 之前的轨道数据显示SPA盆地的地质矿物, 但它们的起源和地质背景尚不清楚.
研究的目的:
- 调查SPA盆地内的卡曼坑的地形材料的组成和起源.
- 分析月球表面的矿物质.
- 评估观察到的矿物质的潜在地幔起源及其地质背景.
主要方法:
- 来自Yutu-2探测器上的可见和近红外光谱仪 (VNIS) 的光谱数据分析.
- 解释矿物学特征,专注于和橄.
- 从撞击坑事件中整合光谱数据与地质背景.
主要成果:
- 最初的VNIS光谱观测表明存在低氧和橄.
- 这些矿物质与来自月球地幔的物质一致.
- 地质背景表明这些地幔材料是由芬森撞击坑挖掘并运送到着陆地点.
结论:
- 这些发现提供了SPA盆地的潜在月球地幔材料的证据.
- 在卡尔曼火山口的探索提供了一个独特的机会,
- 进一步的探索对于了解样本的来源,数量和回收潜力至关重要.
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