Ore-forming processes are relatively well understood on Earth, but little is known about mineralization processes on Mars. By applying terrestrial analogs, using data collected from orbital and rover missions and evidence for hydrothermal activity from alteration assemblages, the types and locations of different ore-forming processes have been investigated with the aim of discovering concentrations of mineral resources on Mars. These resources are likely to be of critical importance for future manned missions to Mars, and insight gained towards mineralization on Mars may also advance our understanding of terrestrial deposits
The Odyssey spacecraft documented the existence of heterogeneously distributed hydrogen at martian m...
One important fraction of the sedimentary record on Mars is composed of evaporite minerals. This rec...
Impact-generated hydrothermal systems have been previously linked to the alteration of Mars’ crust a...
The discovery of phyllosilicates in terrains of Noachian age (>3.5 Ga) on Mars implies a period in t...
Clays form on Earth by near-surface weathering, precipitation in water bodies within basins, hydroth...
Once similarities between Earth and other terrestrial bodies were discovered, determining the condit...
Clays form on Earth by near-surface weathering, precipitation in water bodies within basins, hydroth...
International audienceBasalts are the prevalent rock type on Mars and the products of aqueously alte...
A long-term base on Mars, at the center of an "Exploration Zone", would require substantial quantiti...
As the availability of important mineral deposits on Earth declines, including nuclear minerals, or ...
Over the course of this award we have: 1) Completed and published the results of a study of the effe...
The search for life beyond Earth is the driving motivation for present and planned missions to Mars ...
International audienceAbstract: We focus on processes possibly occurring on Mars that could affect s...
The search for life beyond Earth is the driving motivation for present and planned missions to Mars ...
Due to the high rates of consumption of minerals and the high human population growth, mineral resou...
The Odyssey spacecraft documented the existence of heterogeneously distributed hydrogen at martian m...
One important fraction of the sedimentary record on Mars is composed of evaporite minerals. This rec...
Impact-generated hydrothermal systems have been previously linked to the alteration of Mars’ crust a...
The discovery of phyllosilicates in terrains of Noachian age (>3.5 Ga) on Mars implies a period in t...
Clays form on Earth by near-surface weathering, precipitation in water bodies within basins, hydroth...
Once similarities between Earth and other terrestrial bodies were discovered, determining the condit...
Clays form on Earth by near-surface weathering, precipitation in water bodies within basins, hydroth...
International audienceBasalts are the prevalent rock type on Mars and the products of aqueously alte...
A long-term base on Mars, at the center of an "Exploration Zone", would require substantial quantiti...
As the availability of important mineral deposits on Earth declines, including nuclear minerals, or ...
Over the course of this award we have: 1) Completed and published the results of a study of the effe...
The search for life beyond Earth is the driving motivation for present and planned missions to Mars ...
International audienceAbstract: We focus on processes possibly occurring on Mars that could affect s...
The search for life beyond Earth is the driving motivation for present and planned missions to Mars ...
Due to the high rates of consumption of minerals and the high human population growth, mineral resou...
The Odyssey spacecraft documented the existence of heterogeneously distributed hydrogen at martian m...
One important fraction of the sedimentary record on Mars is composed of evaporite minerals. This rec...
Impact-generated hydrothermal systems have been previously linked to the alteration of Mars’ crust a...