Is ground ice stable near the Martian equator?

Physics

Scientific paper

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Annual Variations, Equators, Evaporation, Evaporation Rate, Land Ice, Mars Surface, Dust, Mars Environment, Polar Regions, Water Vapor

Scientific paper

Determining the present distribution of subsurface water ice on Mars will undoubtedly be a prime objective for future spacecraft missions. Past theoretical studies have predicted that Martian ground ice should be stable to evaporation only at latitudes poleward of approximately +/- 50 deg. Presented here are a new set of calculations which show that bright surficial dust deposits can protect subsurface ice deposits from evaporation at much lower latitudes than previously expected.

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