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Updated: Jun 15, 2025

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
在月球的高度上测量了Chandrayaan-3 APXS的元素丰度
Santosh V Vadawale1, N P S Mithun2, M Shanmugam2
1Physical Research Laboratory (PRL), Ahmedabad, India. santoshv@prl.res.in.
印度
科学领域:
- 月球地质和行星科学.
- 在现场对外星体进行元素分析.
背景情况:
- 月球正流层的组成是了解月球形成和演变的关键.
- 之前的元素组成研究仅限于赤道和中度地区.
- 以往任务的现场测量提供了中度的数据.
研究的目的:
- 报告月球南部高度地区的第一个实地元素丰富度测量.
- 分析月球地形的组成.
- 为遥感观测提供地面真相.
主要方法:
- 在Pragyan探测器上使用阿尔法粒子X射线光谱仪 (APXS) 实验.
- 在Chandrayaan-3着陆地点附近进行了23次现场测量.
- 分析了元素的丰度,重点是铁酸 (FAN) 和黄金物质的指标.
主要成果:
- 在南方高度地区的月球地形在组成上是均的.
- 主要成分是铁酸 (FAN),表明月球岩海洋 (LMO) 的结晶.
- 较高的相对于表明存在混合的物质.
结论:
- 月球南部高度区域的元素成分主要是铁石和石材料的混合物.
- 这一区域的组成均性在几十米内得到证实.
- 这些发现为解释来自月球极地区域的遥感数据提供了宝贵的基础知识.
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