火星の谷の地下水形成は,火星の谷の地下水形成に起因する
1Malin Space Science Systems, San Diego, California 92191-0148, USA. malin@mss.com
Nature
|March 2, 1999
まとめ
地下水は地表の流れではなく,火星の谷のネットワークを形作っている可能性が高い. 高解像度の画像は,地表下の水プロセスがこれらの火星の地質学的特徴を形成する鍵であったことを明らかにします.
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
- 水文学 水文学とは
背景:
- 火星は,古代の洪水に起因する大きな流出チャネルを展示しています.
- 小規模で支流のある谷のネットワークは,論争の的な起源を示しています.
- 既存の仮説には,表面流出 (初期の/後半の火星) または地下水/地下氷のプロセスが含まれています.
研究 の 目的:
- 火星渓谷ネットワークの形成メカニズムを調査する.
- これらの渓谷の形成における地下水の役割を決定する.
- 火星の谷の高解像度の画像を分析するために.
主な方法:
- 火星の谷の高解像度の画像の分析.
- 谷の形状を,既知の地質学的過程と比較する.
主要な成果:
- 高解像度の画像は,谷の形成における地下水の重要な役割を支持しています.
- 証拠によると,地表下の水プロセスが火星の谷の形成に積極的であったことが示唆されています.
- これらの地下水現象の正確なタイミングは不明のままです.
結論:
- 地下水は,火星の渓谷ネットワークの形成に重要な役割を果たしました.
- 表面流出は,これらの渓谷の主要な原因である可能性が低い.
- これらの地下水現象のタイミングを確立するためにさらなる研究が必要である.
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