| Literature DB >> 17844187 |
Abstract
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.Entities:
Year: 1970 PMID: 17844187 DOI: 10.1126/science.168.3934.972
Source DB: PubMed Journal: Science ISSN: 0036-8075 Impact factor: 47.728