まとめ
静寂の海からの月の岩は,最小限の結晶変形を示し,ピロキセンの歪みは,プラスチック流ではなく,急速な冷却に起因する. いくつかの月のシリケートは衝撃変形効果を示します.
科学分野:
- 地質学 地質学 地質学
- ミネラロジーは,鉱物学です.
- 惑星科学は惑星科学である.
背景:
- 静寂の海の結晶岩は,月の地質学的過程についての洞察を提供します.
- 結晶変形メカニズムを理解することは,惑星の進化を解釈する上で極めて重要です.
研究 の 目的:
- 月の岩石におけるプラジオクラゼとオリヴィン結晶の変形メカニズムを調査する.
- ピロキセンの結晶における観測された方向変異の原因を特定する.
- 月面のブレキアとレゴリットにおける衝撃変形の証拠を評価する.
主な方法:
- プラジオクラゼ,オリビン,そしてピロキセンの結晶の顕微鏡検査.
- 結晶の方向転換と変形の特徴の分析.
- 消火した溶融とコンドルールの実験データとの比較.
主要な成果:
- プラジオクラゼとオリヴィン結晶は,静的または動的変形がほとんどまたは全くありません.
- ピロキセンの結晶の方向転換は,プラスチック流ではなく,急速な成長と消火と一致しています.
- 月面のブレキアとレゴリスは,結晶がガラスに変形することを含む,さまざまなレベルの衝撃変形を示します.
結論:
- 観測されたピロキセンの歪みは,月の岩石形成中の急速な冷却プロセスの結果である.
- 衝撃イベントは,月面のいくつかの物質に重大な影響を及ぼし,鉱物の変化を引き起こしました.
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