火星 の 氷河 時代
Isaac B Smith1, Nathaniel E Putzig2, John W Holt3
1Department of Space Studies, Southwest Research Institute, Boulder, CO 80302, USA. isaac@boulder.swri.edu.
まとめ
火星
科学分野:
- 惑星科学
- 気候科学
- 地質学
背景:
- 火星の極地氷は 気候変動の記録を保持しています
- 過去の気候過程を示す 層状の氷の構造を示しています
研究 の 目的:
- 火星の極地氷の観測データを分析する
- 氷の蓄積の歴史と気候サイクルとの関係を理解する
主な方法:
- 火星の極点からのレーダー観測データの詳細分析
- 最後の氷河期以降に蓄積した氷の量の定量化
主要な成果:
- 約8万7千立方キロメートルの氷が 火星の極点に過去37万年に蓄積されています
- この氷の量は およそ60センチメートルの地球層に相当します
- 蓄積された氷のほとんどは 北極に存在します
結論:
- 火星の極地氷は 軌道の周期に関連した 気候の歴史を記録しています
- 結果は過去と将来の火星の気候をモデル化するための制約を提供します.
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