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Simulation of the Planetary Interior Differentiation Processes in the Laboratory
Published on: November 16, 2013
火星のメリディアニ・プランウムで岩床のダイアゲネシスのための火山環境
Thomas M McCollom1, Brian M Hynek
1Center for Astrobiology, University of Colorado, Boulder, Colorado 80309, USA. mccollom@lasp.colorado.edu
Nature
|December 24, 2005
まとめ
メリディアニ・プラヌムの岩床は,浅い塩水からではなく,火山灰がフーマロリック蒸気と反応して形成された可能性が高い. この新しいモデルは,かつて考えられていたよりも,古代の火星の環境が住める可能性が低いことを示唆しています.
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
- 天体生物学 アストロバイオロジー
背景:
- メリディアニ・プラヌムの岩盤には,ヘマタイトや硫酸塩などの鉱物が含まれています.
- 以前の解釈では,蒸発または酸性鉱山排水のような気象による塩水での堆積が示唆されていた.
- これらのモデルは,観測された岩石化学と完全に一致しなかった.
研究 の 目的:
- メリディアニ・プランウムの岩盤の代替的ダイアゲネシスモデルを提案する.
- 観測された鉱物学と化学を,広範囲にわたる地表水を必要とせずに説明するために.
- メリディアニ・プランウム (Meridiani Planum) の古代火星環境の居住可能性を再評価する.
主な方法:
- メリディアニ・プランウム (Meridiani Planum) の岩盤からの化学および鉱物学的証拠の分析.
- 火山灰とフーマロル蒸気を含むダイアゲネティックモデルの開発.
- 提案されたモデルと以前の解釈の比較.
主要な成果:
- 化学組成は浅水または酸性鉱山排水モデルと矛盾しています.
- 火山灰が二酸化硫黄と水を含有する煙気蒸気と反応する代替モデルが提案されています.
- このプロセスは高温で発生し,長期間の地表水の相互作用を必要としない.
結論:
- メリディアニ・プラヌムの岩盤は,おそらく,火山灰のダイアゲネシスによって,フマラロールガスによって形成された.
- この形成シナリオは,以前に推論されたよりも過去の生物学的活動に不利な環境を示唆しています.
- 水と岩の相互作用と初期の火星の居住可能性についての理解を修正する.
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