火星のエンデヴァーブクレーター (エンデヴァーブクレーター) の古代水性環境
R E Arvidson1, S W Squyres, J F Bell
1Department of Earth and Planetary Sciences, Washington University in Saint Louis, St. Louis, MO 63130, USA.
まとめ
オポチュニティ・ローバーは,エンデバークレーターで過去の水と岩の相互作用の証拠を発見し,潜在的に居住可能な環境を明らかにしました. 岩は,生命の初期に有利なわずかに酸性から中性的なpH条件を示しています.
科学分野:
- 惑星科学は惑星科学である.
- 天体生物学 アストロバイオロジー
- 地質学 地質学 地質学
背景:
- Endeavourクレーター・リムには,ノアヒア時代の岩石が含まれています.
- 軌道のスペクトルシグネチャは,鉄 (Fe(+3)) に富んだスメクタイトの存在を示唆しています.
研究 の 目的:
- Endeavourクレーター縁の地質史と岩の水性変化を調査する.
- 過去の水性環境の居住可能性を評価する.
主な方法:
- 軌道スペクトルの反射率分析.
- 岩石の断層のインサイト組成分析.
- 地質的地図作成と層図分析.
主要な成果:
- 識別された細粒子の層状の岩は,球状で,ブレキアで覆われています.
- 衝突後の流体循環を示唆する硫酸カルシウム静脈が検出されました.
- 骨折における水性浸出によるAl豊富なスメクタイト形成の証拠.
- 過去の水と岩の相互作用を推測した,わずかに酸性から中性程度のpH環境.
結論:
- エンデヴァーククレーター・リムには,大きな衝突イベントの前と後の,水と岩の相互作用の証拠が保存されています.
- これらの古代の水性環境は,硫酸塩が豊富な若い場所よりも,潜在的にプレバイオティック化学と微生物生命に有利であった.
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