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月面での22億年の KREEP 豊富な火山活動
Mu-Han Yang1, Qian W L Zhang2, Qiu-Li Li1
1State Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100029, China; College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100049, China.
Science bulletin
|September 3, 2025
まとめ
最新の月の隕石は,KREEP (カリウム,希土元素,リン) の長時間マグマティズムを明らかにし,その期間を8億年延長しました. これは月面マントルの過程が 月の火山の火山を燃やしたことを示唆しています
科学分野:
- 月の地質学
- 同位体地化学
- 惑星科学
背景:
- 月のKREEP成分は火山活動のための主要な熱源です.
- チャンゲーミッションのデータでは クリープの火山活動が疑われる
研究 の 目的:
- 月のKREEP関連マグマティズムの持続時間と源を調べる.
- 最新の月の隕石を分析して 後期火山活動を理解する
主な方法:
- 月の隕石NWA16286の地化学と地年代分析
- 月面ベースルトからの同位体データの収集と分析.
主要な成果:
- NWA 16286は,2億201万年±1300万年前のもので,KREEPに富んだマントルの源を示している.
- これはKREEPに関連するマグマティズムを約8億年延長します.
- 月面の玄武岩は3つの火山のエピソードを示し,U/Pbが増加し,Ndの同位体が減少し,マントルのコンベクションを示している.
結論:
- 月面のマントルの転覆や 噴出によって月面の火山が起きました
- KREEPの成分は,若い火山のエピソード中にベースルトの源にますます組み込まれました.
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