マイクロテクタイト,マイクロクリスタイト,スピネルは,南洋におけるプレオセンの後の小惑星の衝突によるものです
まとめ
太平洋南東部のプレオセンの終わりの小惑星衝突からのガラスの球体は,マイクロテクタイトとマイクロクリスタイトに似ています. そのマグネシオフェライト・スピネルの挿入は,クレタセアス・テリシアル境界の衝突残骸に似た衝撃蒸気から形成されたことを示唆している.
科学分野:
- 地質学 地質学 地質学
- 惑星科学は惑星科学である.
- 堆積物学 堆積物学 堆積物学 堆積物学 堆積物学
背景:
- ガラスのような球体は,堆積物の堆積物の中に存在します.
- これらの球体は小惑星の衝突と関連しています.
- マイクロテクタイトとマイクロクリスタイトの区別は難しいかもしれません.
研究 の 目的:
- プレオセンの後の小惑星の衝突によるガラスの球体の性質を特徴づけるために.
- これらの球粒を,既知のマイクロテクタイトやマイクロクリスタイトと比較する.
- 衝突球体の形成条件を理解する.
主な方法:
- プレオセンの終わりの沈殿堆積物からのガラスの球体の分析.
- スフェルル属性の比較とマイクロテクタイトとマイクロクリスタイトに関する既存のデータ.
- スフェルルインクルージョンの顕微鏡および化学分析.
主要な成果:
- プレオセンの後半の衝突からの球体は,マイクロテクトイトとマイクロクリスタイトの両方に類似した性質を示しています.
- これらの球体は,衝突で発生した蒸気雲からの融解したシリケート滴から形成された可能性が高い.
- マグネシオフェライト・スピネルのインクルージョンが特定され,クレタセウス時代と第三期の境界の衝突球体で見つかったものと類似しています.
結論:
- 研究された球粒は,衝突の残骸であると確認されています.
- これらのプレオセンの後半の球球の形成条件は,白亜紀と地質期の境界の条件に類似していました.
- インパクトイベントは,異なる時代の異なる特徴を持つ異なる地質学的マーカーを作成します.
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