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Schaefer 1990
Schaefer, M.W. (1990). Geochemical evolution of the northern Plains of Mars: Early hydrosphere, carbonate development, and present morphology. Journal of Geophysical Research 95. doi: 10.1029/90JB00571. issn: 0148-0227.

It is likely that early in Mars' history, abundant liquid water was available. Under a thick (several bars) carbon dioxide atmosphere, this water could have formed an ocean, located primarily in the lowlands of the northern hemisphere. An equilibrium geochemical model of this ocean and its interactions with the atmosphere and regolith of Mars was developed, and the results of this model were used to discuss the evolution of the volatile budget of Mars, including the deposition of large carbonate beds on the northern plains. Differential solutional weathering of these carbonate beds may have caused the formation of some of the enigmatic features seen on the northern plains of Mars, such as the thumbprint terrain and enclosed depressions. ¿ American Geophysical Union 1990

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Abstract

Keywords
Planetology, Solid Surface Planets, Composition, Planetology, Solid Surface Planets, Surface materials and properties
Journal
Journal of Geophysical Research
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Publisher
American Geophysical Union
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