Chang'E-3ミッションによって明らかにされた北のマール・インブリウム (Mare Imbrium) の若い多層のテランです
Long Xiao1, Peimin Zhu2, Guangyou Fang3
1China University of Geosciences, Wuhan 430074, China. Macau University of Science and Technology, Macau, China. longxiao@cug.edu.cn zhupm@cug.edu.cn gyfang@mail.ie.ac.cn.
まとめ
中国のChang'E-3ミッションは,月のマールインブリウムに着陸し,複雑な地質学とユニークな岩石の組成を明らかにしました. ユトゥー・ローバーは,これまでサンプリングされていないこの月面地域に関する初期データを提供した.
科学分野:
- 月面地質学 月面地質学
- 惑星科学は惑星科学である.
- 宇宙探査 (宇宙探査) とは,宇宙探査のことです.
背景:
- 中国のChang'E-3ミッションは,以前は直接サンプル採取ができなかった月面地域である北のマール・インブリウムを標的にした.
- 着陸地は,若い450メートルのクレーターの縁に位置しています.
研究 の 目的:
- マール・インブリウムにあるチャンエ3の着陸場所の予備地質学的分析を行うために.
- 地域の地表と地下の組成と地質の歴史を特徴づける.
主な方法:
- チャンエ3着陸機の降下カメラからのデータの分析.
- ユトゥー・ローバーのカメラから撮った画像を用いて.
- ユトゥーローバーの月面浸透レーダー (LPR) のデータを解釈する.
主要な成果:
- ユトゥー・ローバーは114メートルを横断し,掘り起こされた岩石で荒れた表面を記録しました.
- 岩石の分析は,プラジオクラゼとマフィカルシリケート集積物が豊富な組成を示唆し,陸上のドレライトに似ている.
- Lunar Penetrating Radarは,9つの異なる地下層を特定し,複雑な地質学的プロセスを示しています.
結論:
- マール・インブリウム着陸地は,以前のアポロ・ミッションとルナ・ミッションとは異なる地質学的な歴史を示しています.
- この地域の地下構造は,インブリア時代以来の重要な地質進化を示しています.
- 予備的な調査結果は,Chang'E-3着陸地帯のユニークな地質的性質を強調しています.
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