火星のゲールクレーターでChemCamによって観測された土壌の多様性と水分化
P-Y Meslin1, O Gasnault, O Forni
1Université de Toulouse, UPS-OMP, IRAP, 31028 Toulouse, France. pmeslin@irap.omp.eu
まとめ
キュリオシティ・ローバーは,
科学分野:
- 惑星科学は惑星科学である.
- アストロジオロジー アストロジオロジー
- 地質化学 地質化学
背景:
- 火星探査は,土壌の組成を理解することに依存しています.
- 過去の軌道探査は,火星の地球表面の水分化を示していた.
研究 の 目的:
- 火星の土壌の種類とその水分を特徴づけるために.
- 火星のレゴリットと大気の相互作用を調査する.
主な方法:
- 火星の土壌の化学をChemCam機器でインシット分析した.
- 土壌サンプルのスペクトル解析.
- データの相関関係とチェミン・インストゥルメントの調査結果.
主要な成果:
- 2つの主要な土壌タイプが特定されました:細粒子のマフィスと粗粒子のフェルシックスです.
- マフィックの土壌は,火星の塵に似ているが,一貫した水素のサインを示している.
- この水分補給は,無形土壌相と関連しており,地球表面の水分補給に大きく貢献しています.
結論:
- 火星のマフィック土壌は水分化されており,おそらく無形相によるものです.
- レゴリットと大気間の有意な水蒸気交換は検出されなかった.
- 発見は,アモルフな相の性質と火星の水分補給におけるその役割を制限する.
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