Abstract
Martian gullies have been seen as evidence for past surface water runoff. However, numerical modelling now suggests that accumulation and sublimation of carbon dioxide ice, rather than overland flow of liquid water, may be driving modern gully formation.
Cite
CITATION STYLE
APA
Dundas, C. (2016). Mars on dry ice. Nature Geoscience, 9(1), 10–11. https://doi.org/10.1038/ngeo2625
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