火星で観測されたメタンの変動は,既知の大気化学と物理によって説明できない
Franck Lefèvre1, François Forget
1LATMOS, UPMC Université Paris 06, CNRS, Paris 75005, France. franck.lefevre@upmc.fr
Nature
|August 8, 2009
まとめ
火星のメタンは季節的な変化を示していますが,現在のモデルはこれを説明できません. より速いメタンの損失プロセスが必要であり,それは有機的な生存に不適した厳しい火星環境を示唆しています.
科学分野:
- 惑星科学は惑星科学である.
- 天体生物学 アストロバイオロジー
- 大気化学 大気化学
背景:
- 火星でのメタンの検出は,過去/現存する生命とアビオジェニックの起源についての議論を助長しています.
- 観測されたメタンの濃度は,局所的な増強と季節的な変動を示し,その長い光化学寿命と矛盾しています.
研究 の 目的:
- 火星で観測されたメタンの変動が,メタン化学に関する我々の理解に及ぼす影響を調査する.
- 観測されたメタンダイナミクスと現在の光化学モデルの間の不一致を調和させるため.
主な方法:
- 火星の地球気候モデルと化学の組み合わせを用いた.
- メタンの分布に対する光化学と二酸化炭素濃縮-亜鉛化サイクルの影響を調査した.
- 大気中の寿命要件を評価するために,メタンの放出シナリオをシミュレートします.
主要な成果:
- 標準的な光化学は,局所的でエピソード的な放出であっても,観測されたメタンの変動を説明することはできません.
- 二酸化炭素濃縮-亜鉛化サイクルは,大規模なメタンの変動を生成しますが,観測されたパターンには一致しません.
- 局所的なメタンの増強を複製するには,大気中の寿命が200日未満で,未知で急速なメタンの損失プロセスを意味する.
結論:
- 火星のメタン化学の現在の理解は不完全である.
- 観測を説明するために,予測よりも著しく速い,未確認のメタン喪失プロセスが必要である.
- 確認された場合,これらの変異は,有機的な生存に有害な厳しい火星表面環境を示唆します.
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