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- Andrew P. Ingersoll
- Division of Geological Sciences, California Institute of Technology, Pasadena 91109
書誌事項
- 公開日
- 1970-05-22
- DOI
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- 10.1126/science.168.3934.972
- 公開者
- American Association for the Advancement of Science (AAAS)
この論文をさがす
説明
<jats:p>In the absence of juvenile liquid water, condensation of water vapor to ice and subsequent melting of ice are the only means of producing liquid water on the martian surface. However, the evaporation rate is so high that the available heat sources cannot melt pure ice. Liquid water is therefore limited to concentrated solutions of strongly deliquescent salts.</jats:p>
収録刊行物
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- Science
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Science 168 (3934), 972-973, 1970-05-22
American Association for the Advancement of Science (AAAS)