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マグネシウム硫酸塩と火星の水の歴史

David T Vaniman1, David L Bish, Steve J Chipera

  • 1Los Alamos National Laboratory (LANL), MS D462, Los Alamos, New Mexico 87545, USA. vaniman@lanl.gov

Nature
|October 8, 2004
PubMed
まとめ

火星上の硫酸マグネシウムの塩は,かなりの量の水を保持することができ,観測された赤道水を潜在的に説明します. 彼らの水分状態は,温度と湿度に敏感であり,正確な火星の水の歴史評価のためにインサイト分析が必要です.

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