38Ar/36Arの上層大気測定から得られた火星の大気史
B M Jakosky1, M Slipski2, M Benna3
1University of Colorado, Boulder, CO, USA. bruce.jakosky@lasp.colorado.edu.
まとめ
火星は大気中のアルゴンの66%を 宇宙に失いました 大気中のガスの減少は 惑星が
科学分野:
- 惑星科学
- 大気科学
- 天体生物学
背景:
- 火星の大気の歴史を理解することは,その地質学的進化と過去の居住可能性を評価するために不可欠です.
- 温暖で湿った初期の火星から 現在の冷たく乾燥した状態への移行は 大気の損失と関連しています
研究 の 目的:
- 時間の経過とともに 宇宙に失われた大気ガスの量を 定量化するためです
- 火星の大気逃亡を 駆動するメカニズムを調査するためです
主な方法:
- 火星大気と揮発性進化 (MAVEN) 宇宙船からのデータを使用した.
- 上層大気構造を分析した 特に38Ar/36Ar同位体の比率
- ホモパウズとエクソベースの高さ間のアルゴン同位体構造を導出した.
主要な成果:
- 軽いイソトープの損失によるアルゴンイソトープの有意な分断を決定した.
- 火星の大気中のアルゴンの66%が 宇宙に失われていると計算しました
- 大気逃亡と火星の気候の進化の間の直接的なリンクを確立しました
結論:
- 火星の大気の大部分は 宇宙に逃げた.
- 火星の大気汚染は 火星の大気変動の 重要な要因です
- この研究は 過去の火星の居住可能性について 重要な洞察を与えてくれます
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