Add to ORKGModern climate models of Mars tend to predict a colder, icier early climate than previously imagined. While alteration of mafic terrain under warm, wet conditions is relatively well understood, a significant knowledge gap exists in how weathering might occur under redominantly glaciated environments on Mars. In such conditions, it is unclear whether all or any of the variety of aqueous alteration phases expressed in contemporaneous early martian surfaces could be formed, or how erosion of mafic bedrock and transport of sediment would comparatively change. Please see attachment
abstract: Amorphous phases are detected over large regions of the Martian surface from orbit and in ...
Terrestrial weathering processes in cold-desert climates such as the Dry Valleys of Antarctica may p...
abstract: Chemical and physical interactions of flowing ice and rock have inexorably shaped planetar...
Liquid water was abundant on early Mars, but whether the climate was warm and wet or cold and icy wi...
The bulk of the Martian crust is basaltic with a wide variety of subsequently derived aqueous altera...
Although the current cold, dry environment of Mars extends back through much of its history, its ear...
Geomorphological and mineralogical data from early Martian surfaces indicate liquid water was presen...
Geologic evidence suggests that the surface of Mars has been dominated by cold, dry, and relatively ...
Surface weathering on Earth is driven by precipitation (rain/snow melt). Here we summarize the influ...
Liquid water was abundant on early Mars, but whether the climate was warm and wet or cold and icy wi...
Soil crystallinity is largely determined by leaching rates, as high leaching rates favor the rapid p...
A model for the formation and distribution of sedimentary rocks on Mars is proposed. In this model (...
Many geomorphic features on Mars were attributed to Earth-analogous, cold-climate processes involvin...
While ancient fluvial channels have long been considered strong evidence for early surface water on ...
Primary objectives for exploration of Mars include determination of: (1) the distribution, abundance...
abstract: Amorphous phases are detected over large regions of the Martian surface from orbit and in ...
Terrestrial weathering processes in cold-desert climates such as the Dry Valleys of Antarctica may p...
abstract: Chemical and physical interactions of flowing ice and rock have inexorably shaped planetar...
Liquid water was abundant on early Mars, but whether the climate was warm and wet or cold and icy wi...
The bulk of the Martian crust is basaltic with a wide variety of subsequently derived aqueous altera...
Although the current cold, dry environment of Mars extends back through much of its history, its ear...
Geomorphological and mineralogical data from early Martian surfaces indicate liquid water was presen...
Geologic evidence suggests that the surface of Mars has been dominated by cold, dry, and relatively ...
Surface weathering on Earth is driven by precipitation (rain/snow melt). Here we summarize the influ...
Liquid water was abundant on early Mars, but whether the climate was warm and wet or cold and icy wi...
Soil crystallinity is largely determined by leaching rates, as high leaching rates favor the rapid p...
A model for the formation and distribution of sedimentary rocks on Mars is proposed. In this model (...
Many geomorphic features on Mars were attributed to Earth-analogous, cold-climate processes involvin...
While ancient fluvial channels have long been considered strong evidence for early surface water on ...
Primary objectives for exploration of Mars include determination of: (1) the distribution, abundance...
abstract: Amorphous phases are detected over large regions of the Martian surface from orbit and in ...
Terrestrial weathering processes in cold-desert climates such as the Dry Valleys of Antarctica may p...
abstract: Chemical and physical interactions of flowing ice and rock have inexorably shaped planetar...