Abstract
In order to better understand the stability of water on Mars, and factors likely to affect that stability, we have measured the evaporation rate of water in a CO2 atmosphere at 7 mbar and ∼0°C in a large environmental chamber that minimizes fluctuation in conditions. The average evaporation rate we measured was 1.01 ± 0.19 mm/h. This includes correction for water vapor build-up in the chamber, but not the effect of Mars' lower gravity. When corrections for this are applied, our predicted evaporation rate for water on Mars at 0°C and 7 mbar is 0.73 ± 0.14 mm/h. This is in very good agreement with the value calculated by assuming that evaporation depends on diffusion and buoyancy. The consistency of these results suggests that - at least for these conditions - our approaches to the calculations and the laboratory simulations are reasonable. Copyright 2005 by the American Geophysical Union.
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CITATION STYLE
Sears, D. W. G., & Moore, S. R. (2005). On laboratory simulation and the evaporation rate of water on Mars. Geophysical Research Letters, 32(16), 1–4. https://doi.org/10.1029/2005GL023443
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