オポチュニティ・ローバーの着陸地にあるイーグル・クレーターとメリディアニ・プラニュムの土壌
L A Soderblom1, R C Anderson, R E Arvidson
1U.S. Geological Survey, Flagstaff, AZ 86001, USA. lsoderblom@usgs.gov
まとめ
火星 火星 火星 火星
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:
- オポチュニティ・ローバーは,メリディアニ・プランウム (Meridiani Planum) の土壌を調査した.
- これらの土壌は,細粒子の玄武岩砂,塵,硫酸塩に富んだ破片で構成されています.
研究 の 目的:
- オポチュニティの場所にある火星の土壌の構成と起源を特徴づけるため.
- メリディアン平面 (Meridiani Planum) を形作る地質学的プロセスを理解する.
主な方法:
- オポチュニティ・ローバーによる土壌と岩石のサンプル分析.
- 顕微鏡画像と元素組成分析.
主要な成果:
- ヘマタイトの球粒は表面に濃縮され,塩化によって掘り起こされます.
- 土壌は塩で覆われ,おそらく地表のセメント化によるものです.
- ヘマタイトに富んだ粒子が装甲したエオリアン波紋は広範囲に広がっています.
- 土層の厚さは約1メートル.
結論:
- 土壌の特徴と地形は,Meridiani Planumが古代の堆積物表面である可能性を示唆しています.
- 塩化とエオリアのプロセスは,表面の改変に重要な役割を果たします.
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