月面の微細粒子のガラスのような粒子は,月面の微細粒子の
1Institute of Molecular Evolution, University of Miami, Coral Gables, Florida 33134, USA.
Nature
|October 17, 1970
まとめ
アポロ11号のガラスの粒子の大半はユニークで,典型的な火山や衝突によって形成されたものではない. 月面上の太陽のフレア活動から,月面のいくつかの月面粒子が発生している可能性があります.
科学分野:
- 月面地質学 月面地質学
- 宇宙科学とは,宇宙の科学である.
- アストロジオロジー アストロジオロジー
背景:
- アポロ11号は,ガラスのような粒子を含めた月面サンプルを回収した.
- 月の粒子の起源を理解することは,月科学にとって極めて重要です.
- 以前の研究は,陸上の火山活動,隕石の衝突,隕石の親体の凝縮に重点を置いていました.
研究 の 目的:
- アポロ11号のガラスの粒子の起源を区別するために.
- ユニークな月の粒子の潜在的形成メカニズムを調査する.
主な方法:
- アポロ11号のガラスのような粒子の比較分析.
- 火山活動,衝撃,凝縮による形成過程の調査.
- 月のレゴリットとの太陽フレアの相互作用の検討.
主要な成果:
- アポロ11号のガラスの粒子の大部分は,地上の火山や隕石の衝突の起源とは異なる特徴を示しています.
- これらの粒子の大部分は,隕石の親体からの凝縮産物と一致しない.
- 証拠は,月面と太陽フレアの相互作用を含む潜在的な形成経路を示唆しています.
結論:
- アポロ11号のガラスのような粒子は,月のユニークな材料を表しています.
- 太陽フレア活動は,月のいくつかのガラスのような粒子の形成のための妥当なメカニズムです.
- これらのユニークな月のサンプルの起源を完全に解明するには,さらなる研究が必要です.
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