アポロ11号の月のサンプルの炭素化合物
B Nagy1, W M Scott, V Modzeleski
1Department of Geochronology, University of Arizona, Tucson 85721, USA.
Nature
|March 14, 1970
まとめ
この研究では,月の揮発性物質の起源を調査しています. 太陽風,隕石,彗星,原始大気,月面からのガス排出など,潜在的な源を分析して,月面の揮発性インベントリに寄与する要因を特定します.
科学分野:
- 月科学は月科学である.
- 惑星科学は惑星科学である.
- アストロジオロジー アストロジオロジー
背景:
- 月の揮発性成分は完全に理解されていません.
- 月面の揮発性物質の起源について,複数の仮説が存在する.
研究 の 目的:
- 月面の揮発性物質の様々な提案された源を批判的に評価する.
- 月の不安定な在庫への内部と外部からの貢献を区別するために.
主な方法:
- 太陽風の植え付けに関する既存の文献のレビュー.
- 隕石や彗星の物質の同位体組成の分析.
- 月のガス排出過程の地球化学モデリング.
- 観測された月面の揮発性シグネチャと潜在的な源貯蔵庫の比較.
主要な成果:
- 証拠は,月面の揮発性物質の混合起源を示唆しています.
- 太陽風の植え付けは,特定の揮発性元素の重要な源である.
- 隕石や彗星の衝突により,他の揮発性生物種が絶滅した可能性が高い.
- 原始大気残留物と排出ガスも役割があるかもしれない.
結論:
- 月面の揮発性在庫は,複数の配送と形成プロセスの複雑な産物である.
- 確固たる源代を決定するには,さらなる現場測定とサンプル分析が必要である.
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