イエロウナイフ湾,ゲールクレーター,火星の居住可能なフリヴィオ・ラクストリン環境
J P Grotzinger1, D Y Sumner, L C Kah
1Division of Geologic and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA.
まとめ
火星 火星 火星 火星
科学分野:
- 天体生物学 アストロバイオロジー
- 惑星科学は惑星科学である.
- 地質学 地質学 地質学
背景:
- 古代の火星は,生命に潜在的に適した環境を持っていた.
- キュリオシティローバーは,火星の地質学と居住可能性を調査する.
研究 の 目的:
- 火星で過去に居住可能な環境があったという証拠を探すために堆積岩を分析する.
- ケモリトオオートロフィック火星生物圏の可能性を評価する.
主な方法:
- キュリオシティローバーによる細粒子の堆積岩の分析.
- 岩の組成と鉱物学に基づいて推測された環境条件.
主要な成果:
- 古代の湖床の堆積岩を発見した.
- ニュートラルなpH,低塩分,変数のリドックス状態の水性環境の特定.
- 主要な生物学的要素 (C,H,O,S,N) の存在と,推論されたの利用可能性.
結論:
- 火星の河流・湖流の環境は,生物学的に生存可能であった.
- 証拠は,火星のノア紀後の歴史において,持続的な居住可能な環境が存在していたことを示唆しています.
- この発見は,過去の火星生命の存在の可能性を裏付けている.
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