A simple model of local heat transport on Mars demonstrates that transient melting of ice may occur in depressions and gullies nearly anywhere on the planet where thin ice is illuminated by normal-incidence insolation. An experiment has been performed to confirm the model of evaporation rate at low
Liquid water on Mars
β Scribed by Crofton B. Farmer
- Publisher
- Elsevier Science
- Year
- 1976
- Tongue
- English
- Weight
- 842 KB
- Volume
- 28
- Category
- Article
- ISSN
- 0019-1035
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