月面から採集された玄武岩の源に対する同位体および組成上の制約
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.
まとめ
チャンエ6号は南極・アイトケン盆地から 月石を分析した. これらの玄武岩は,月のマグマ海洋 (LMO) の結晶化と,SPAの衝突による潜在的マントルの改変を示唆しています.
科学分野:
- 月の地質学と火山学
- 惑星科学
- 地質年代学
背景:
- 月面の火山は月面内部の過程を理解するために不可欠なベースルト堆積物を生み出しました
- チャンエ6号は,月の反対側にある南極・アイトケン盆地 (SPA) からサンプルを回収した.
研究 の 目的:
- チェンジ6号からの塩基岩の成分と年齢を分析する
- 月面内部のプロセスと月面マグマ海洋 (LMO) モデルに対するこれらの玄武岩の影響を調査する.
主な方法:
- チェンジ6号が収集した ベースルトの断片の分析
- 塩基岩の年齢と源の特徴を決定するためのウラン鉛 (U-Pb) 年代測定.
主要な成果:
- チェンジ6の塩基岩は,低チタンのアポロ塩基岩と組成的に似ている.
- U-Pb年代測定により,ベースルトの年齢は2,823.0 ±590万年であった.
- 高源238U/204Pb比 (μ値) は480±56で,LMOの結晶化が遅れていることを示している.
結論:
- この発見は月のマグマ海洋 (LMO) モデルを支持しますが,アポロのサンプル傾向から逸脱しています.
- Chang'e-6のベースルトデータは,LMO後のマントルの改変を示唆し,SPAの影響と関連している可能性がある.
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