Add to ORKGEvidence is presented for large standing bodies of water on Mars during past epochs. It is noted that the origin of the horizontally-layered deposits in the Valles Marineris can be best explained by formation in standing bodies of water. These lakes, if they existed, were most likely covered by ice. There are several geologically feasible mechanisms that could have led to formation to thick deposits in ice covered paleolakes in the Valles Marineris. Present data are insufficient to choose conclusively among the various possibilities
The current climate of Mars is characterized by annual cycles of carbon dioxide (CO 2 ) and water co...
In this work we estimate the minimum persistence time of subsurface ice in water rich sediment layer...
An extensive layered formation covers the high plateaus around Valles Marineris. Mapping based on Hi...
Thick sequences of layered deposits are found in the Valles Marineris, which exhibit fine, nearly ho...
An important contribution to the volatile history of Mars comes from a study of Valles Marineris, wh...
The problems of how warm and wet Mars once was and when climate transitions may have occurred are no...
The identification of possible shorelines in the Martian northern plains suggests that the water dis...
The surface of Mars is incised with hundreds of ancient valley networks, the physical record of flow...
International audienceLayered deposits are exposed in the walls of the troughs cutting the north pol...
International audienceLayered deposits are exposed in the walls of the troughs cutting the north pol...
Only a few years ago the common notion was that Mars today is a dry place. With the excellent datase...
[1] Geomorphic evidence suggests that recent gullies on Mars were formed by fluvial activity. The Ma...
The poles of Mars are known to have recorded recent (<107 years) climatic changes. While the south p...
The polar layered deposits are thought to contain alternate layers of water and dust in different pr...
Candor Mensa, an interior layered deposit (ILD) in Valles Marineris, Mars, consists of two stratigr...
The current climate of Mars is characterized by annual cycles of carbon dioxide (CO 2 ) and water co...
In this work we estimate the minimum persistence time of subsurface ice in water rich sediment layer...
An extensive layered formation covers the high plateaus around Valles Marineris. Mapping based on Hi...
Thick sequences of layered deposits are found in the Valles Marineris, which exhibit fine, nearly ho...
An important contribution to the volatile history of Mars comes from a study of Valles Marineris, wh...
The problems of how warm and wet Mars once was and when climate transitions may have occurred are no...
The identification of possible shorelines in the Martian northern plains suggests that the water dis...
The surface of Mars is incised with hundreds of ancient valley networks, the physical record of flow...
International audienceLayered deposits are exposed in the walls of the troughs cutting the north pol...
International audienceLayered deposits are exposed in the walls of the troughs cutting the north pol...
Only a few years ago the common notion was that Mars today is a dry place. With the excellent datase...
[1] Geomorphic evidence suggests that recent gullies on Mars were formed by fluvial activity. The Ma...
The poles of Mars are known to have recorded recent (<107 years) climatic changes. While the south p...
The polar layered deposits are thought to contain alternate layers of water and dust in different pr...
Candor Mensa, an interior layered deposit (ILD) in Valles Marineris, Mars, consists of two stratigr...
The current climate of Mars is characterized by annual cycles of carbon dioxide (CO 2 ) and water co...
In this work we estimate the minimum persistence time of subsurface ice in water rich sediment layer...
An extensive layered formation covers the high plateaus around Valles Marineris. Mapping based on Hi...