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Updated: Aug 13, 2026

Chemical Gardens as Flow-through Reactors Simulating Natural Hydrothermal Systems
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火星で水熱カルボネートの形成のための地化学モデル

L L Griffith1, E L Shock

  • 1Department of Earth and Planetary Sciences, McDonnell Center for the Space Sciences, Washington University, St. Louis, Missouri 63130, USA.

Nature
|October 5, 1995
PubMed
まとめ

火星は,かなりの量の二酸化炭素と水を失っているかもしれない. 水熱カルボネートは,これらの揮発性物質が火星の表面の下に閉じ込められている可能性の合理的な説明を提供します.

キーワード:
NASAの規律 エクゾバイオロジー非NASAのセンターです.

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