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Updated: Jun 7, 2025

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Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
Published on: July 30, 2020
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28億年前の月面の火山活動 6の玄武岩
Qian W L Zhang1, Mu-Han Yang1,2, Qiu-Li Li3,4
1State Key Laboratory of Lithospheric and Environmental Coevolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing, China.
Nature
|November 15, 2024
まとめ
月面の遠方の火山は14億年以上にわたって持続し,サンプルでは42億年前のKREEP豊富な源と,若いベースルトのKREEPの少ない源を明らかにしました. フォースサイド・クレーター・クロノロジー・モデルと一致する
科学分野:
- 月の地質学
- 惑星科学
- 地質年代学
背景:
- 月の火山の歴史を理解することは 半球間の違いを説明する鍵です
- 過去の研究では,クレーター形成に基づいた長寿の遠端火山活動が示唆されたが,サンプル証拠は欠けていた.
研究 の 目的:
- 月面の火山の歴史を調査する
- 月面のクレーター年代測定モデルを検証し 精査する
主な方法:
- チェンジ6号が帰還したベースルトのPb-Pb年代測定
- 源の特性 (μ値) を決定するためのU-Pb同位体組成の分析.
主要な成果:
- KREEPが豊富な源から4,203 ± 4 マ (最古の返還サンプル) と,KREEPが少ない源から2,807 ± 3 マのエピソードが特定されました.
- 若い火山の年齢はクレーターカウントの推定値と一致し,遠くのクロノロジーモデルを検証します.
- 月の裏側での火山活動が 14億年以上続いたことを証明しました
結論:
- 月面の遠方の火山は長生きし,KREEPが豊富からKREEPが少ない源へと進化した.
- 遠方の火山の歴史に 重要なサンプルを 提供した.
- クレーター年代記モデルは,月の両半球に適用できます.
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