初期の火星は二酸化炭素の雲で暖められ,赤外線を散乱させる
1Laboratoire de Météorologie Dynamique du CNRS, Université Pierre et Marie Curie, Boite Postale 99, 4 place Jussieu, 75252 Paris Cedex 05, France. forget@lmd.jussieu.fr
まとめ
初期の火星は,二酸化炭素の氷雲が熱を反射し,古代の流れる水の謎を解いて温暖化していたのかもしれない. この温室効果の変種は,地球の初期の気候や系外惑星の居住可能なゾーンについても説明できる.
科学分野:
- 惑星科学は惑星科学である.
- 気候モデリング
- 天体生物学 アストロバイオロジー
背景:
- 地形的な証拠によると,火星には38億年前に液体の水が存在していた.
- 従来の温室効果温暖化モデルは,火星の初期の温暖化を説明できない.
研究 の 目的:
- 初期の火星の代替的な温暖化メカニズムを調査する.
- 初期の地球と系外惑星の居住可能性への影響を調査する.
主な方法:
- 二酸化炭素の氷雲を通る放射性伝達のモデル計算.
- 散布による温室効果メカニズムの分析.
主要な成果:
- 二酸化炭素の氷の雲は,散布温室効果を生じさせる可能性があります.
- このメカニズムは,初期の火星を液体の水のために十分に温めることができます.
- このプロセスは,初期の地球の気候と太陽系外惑星の居住可能なゾーンの説明を提供します.
結論:
- 二酸化炭素の氷の雲による散布温室効果は,火星の初期の温暖化についての合理的な説明である.
- このメカニズムは,惑星の居住可能性についてより広範な意味を持つ.
- 雲と気候の相互作用に関するさらなる研究が必要である.
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