火星上のヘマタイトの具体化に対する地球上の類似点である可能性がある
Marjorie A Chan1, Brenda Beitler, W T Parry
1Department of Geology and Geophysics, University of Utah, 135 S 1460 E, Salt Lake City, Utah 84112-0111, USA. machan@mines.utah.edu
Nature
|June 18, 2004
まとめ
火星の球状のヘマタイト凝固は,ユタ州で見つかったものと類似しています.
科学分野:
- 惑星科学 惑星科学
- 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:
- 火星の探査は,その浅い地表の地下で水に富んだ過去の証拠を明らかにしています.
- Meridiani Planumで見つかったヘマタイトに富んだ球状の凝固は,地上のダイアゲネティック凝固に似ている.
研究 の 目的:
- 火星のコンクリエーションをナバホー砂岩からの地上の類似物と比較するために.
- 火星における地下水関連の形成メカニズムに類似したものを調査する.
主な方法:
- 火星とナバホ・サンドストーンからの球形の凝固の比較分析.
- 地上コンクリートの特徴に基づく宿主岩の性質と流体プロセスの推論.
主要な成果:
- 火星と地上のコンクリエーションは,驚くべき形態学的および組成的な類似性を共有しています.
- 火星上のこれらの球形コンクリエーションの形成は,特定の地質学的条件を暗示しています.
結論:
- 浸透性宿主岩,地下水の流れ,化学反応フロントの存在は,火星のコンクリート形成に不可欠であると推論されています.
- これらの発見は,火星の過去の地下水の活動に関する仮説を裏付けている.
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