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シェルゴッティ隕石のシリカのモノクリニック・ポスト・スティシュホイット・ポリモルフ
El Goresy A1, Dubrovinsky, Sharp
1Max-Planck-Institut fur Chemie, J.-Becher-Weg 27, D-55128 Mainz, Germany. Theoretical Geochemistry Program, Institute of Earth Sciences, Uppsala University, S-75236, Uppsala, Sweden. Department of Geology, Arizona State University, Tempe, A.
まとめ
研究者らは,シェルゴッティの隕石で,スタイショバイト後の新種のシリカ相を特定した. この発見は,地外的な衝撃イベントの間に形成された高圧シリカポリモルフに関する新しい洞察を提供します.
科学分野:
- ミネラロジーは,鉱物学です.
- 惑星科学は惑星科学である.
- マテリアルサイエンス 材料科学
背景:
- 隕石は,惑星の過程を理解するために重要なサンプルを提供します.
- シリカは,stishoviteを含む多様な高圧ポリモルフを示しています.
- 衝撃イベントは,隕石の極端な圧力と温度条件を誘導することができます.
研究 の 目的:
- シェルゴッティ隕石の高圧シリカ相を特定し,特徴づけること.
- ショックイベントの結果生じる鉱物学的変容を調査する.
主な方法:
- 結晶学的分析のためのX線微分法 (XRD).
- 微細構造調査のためのフィールドエミッションスキャニング電子顕微鏡 (FESEM).
- 詳細なフェーズ識別のための伝送電子顕微鏡 (TEM).
主要な成果:
- モノクリニックの格子を持つステシュホイット後シリカ相の識別.
- ユニットセルパラメータの特徴と,新しいフェーズの密度.
- 同じシリカ粒の内部にあるスティショバイトとクリストバライトの観測により,複数の高密度ポリモルフが示された.
結論:
- シェルゴッティ隕石には,これまで未確認のポストステシュホイットシリカポリモルフが含まれています.
- 複数の高密度シリカ相の存在は,衝撃変形過程における複雑な変容を示唆する.
- この発見は,極端な地球外環境下でのシリカの振る舞いの理解に寄与しています.
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