ニュートロン誘発によるウランの分裂:月の表面物質の年代測定方法
まとめ
アポロ17号の火山ガラスは363億年前に形成され,月の表面で3800万年過ごしました. 後に埋葬され,1700万年前のショーリークレーター衝突で再発掘された.
科学分野:
- 月面地質学 月面地質学
- 宇宙化学 (コスモケミストリー)
- ジオクロノロジー (Geochronology) について
背景:
- アポロ17号はショルティクレーターから火山ガラスを収集した.
- これらのメガネは,月面のプロセスと月面の歴史についての洞察を提供します.
研究 の 目的:
- アポロ17号からの火山のメガネの年齢と表面被曝歴を決定する.
- これらのサンプルに影響を与える地質学的出来事を再構築するために.
主な方法:
- クセノン-136同位体の分析.
- 火山ガラスの放射線年代測定.
- ウラン235のニュートロン誘発分裂測定.
主要な成果:
- 火山のガラスは3630億年前に形成されました.
- サンプルは,3800万年の表面被曝を経験した.
- 再発掘は1700万年前にショルティクレーター衝突により発生した.
結論:
- この研究は,アポロ17号の火山ガラスの詳細なタイムラインを確立しています.
- 月面曝露と埋葬/再発掘の出来事が定量化されています.
- 月の衝撃と地質史を理解するための重要なデータを提供します.
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