Mars: Occurrence of Liquid Water

  • Andrew P. Ingersoll
    Division of Geological Sciences, California Institute of Technology, Pasadena 91109

書誌事項

公開日
1970-05-22
DOI
  • 10.1126/science.168.3934.972
公開者
American Association for the Advancement of Science (AAAS)

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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>

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  • Science

    Science 168 (3934), 972-973, 1970-05-22

    American Association for the Advancement of Science (AAAS)

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