火星の南部の高地における塩素含有物質
M M Osterloo1, V E Hamilton, J L Bandfield
1Hawaii Institute of Geophysics and Planetology, University of Hawaii, 1680 East-West Road, Honolulu, HI 96822, USA. osterloo@higp.hawaii.edu
まとめ
火星 火星 火星 火星
科学分野:
- 惑星科学は惑星科学である.
- 地質学 地質学 地質学
- 天体生物学 アストロバイオロジー
背景:
- 塩化物は,水の蒸発と火山活動によって形成されます.
- 火星の表面積は,塩化物を含有する物質の存在を示唆している.
研究 の 目的:
- 火星の塩化物堆積地を特定し,地図化するために.
- これらの堆積物の地質的文脈と影響を理解する.
主な方法:
- 火星オデッセイ熱放出画像システム (THEMIS) のデータを活用した.
- 軌道上の画像からのスペクトルサインと地形学的特徴を分析した.
主要な成果:
- 識別されたスペクトル的に明確な,明るい色調の,多角的に割れた塩化物堆積物.
- 堆積物は,南部の高原の低アルベド地域,主にノアキアの地形で広く見られる.
結論:
- クロリドの存在は,火星の表面近くで水が存在していたことを示している.
- これらの発見は,湿った初期の火星の歴史の理論を支持します.
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