火星の近地における水素の分布:地下の氷の堆積物の証拠
W V Boynton1, W C Feldman, S W Squyres
1Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA. wboynton@lpl.arizona.edu
まとめ
マース・オデッセイ マース・オデッセイ
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
- 地質学 地質学 地質学
背景:
- 火星には極地の氷蓋があるが,地表下の氷の範囲と構成は,現在も活発な研究の対象となっている.
- 水素の分布を理解することは,火星の過去の居住可能性と水資源の可能性を評価するための鍵です.
研究 の 目的:
- 軌道データを用いて火星の水素に富んだ地下の地域を特定し,特徴づけること.
- これらの水素堆積物の組成と物理的状態を調査する.
主な方法:
- Mars Odyssey軌道に乗ったガンマ線スペクトロメーターのデータを活用した.
- 緯度と氷の安定性ゾーンに関する水素の分布と柱の密度を分析し,氷の安定性ゾーンを予測した.
主要な成果:
- 地下水素濃縮が顕著な2つの異なる極域を特定した.
- ポールに向かって,水素が少ない層の厚さの減少が観察されました.
- 水素が豊富な層は,水の氷が安定すると予測された領域と強い相関関係を示した.
結論:
- 地下水素は,水氷の形であり,濃縮層の重量の約35%を占めています.
- これらの発見は,火星の極緯度で,かなりの地下氷堆積物の存在を裏付けている.
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