© 2015 The Authors.Near-infrared remote sensing data of Mars have revealed thousands of ancient deposits of Fe/Mg-rich smectitic clay minerals within the crust with relevance to past habitability. Diagnostic metal-OH infrared spectroscopic absorptions used to interpret the mineralogy of these phyllosilicates occur at wavelengths of 2.27-2.32 μm, indicating variable Fe/Mg ratios in the clay structures. The objective of this work is to use these near infrared absorptions to constrain the mineralogy of smectites on Mars. Using Fe/Mg-rich seafloor clay minerals as mineralogical and spectroscopic analogs for Martian clay minerals, we show how crystal-chemical substitution and mixed layering affect the position of the diagnostic metal-OH spectral...
Seafloor hydrothermal sites generate abundant Mg- and Fe-rich clays. These clays are structurally an...
To understand the aqueous history of Mars, it is critical to constrain the alteration mineralogy of ...
Ferric (Fe3+-bearing) smectites, including nontronite, constitute the majority of hydrous mineral ex...
Near-infrared remote sensing data of Mars have revealed thousands of ancient deposits of Fe/Mg-rich ...
AbstractNear-infrared remote sensing data of Mars have revealed thousands of ancient deposits of Fe/...
Aqueous alteration on Mars can produce a range of tell-tale secondary minerals [1]. Surface missions...
During its exploration of the Columbia Hills, the Mars Exploration Rover ‘‘Spirit’...
Aluminous clay deposits on Mars are recognized from remotely sensed infrared spectral features simil...
Clay minerals provide indicators of the evolution of aqueous conditions and possible habitats for li...
One of the primary science goals of Mars Science Laboratory (MSL) is to investigate layered clay min...
Clays form on Earth by near-surface weathering, precipitation in water bodies within basins, hydroth...
The search for life beyond Earth is the driving motivation for present and planned missions to Mars ...
The Noachian terrain west of the Isidis basin hosts a diverse collection of alteration minerals in r...
Clays form on Earth by near-surface weathering, precipitation in water bodies within basins, hydroth...
This dissertation is comprised of three studies investigating clay mineralogy on, or near the martia...
Seafloor hydrothermal sites generate abundant Mg- and Fe-rich clays. These clays are structurally an...
To understand the aqueous history of Mars, it is critical to constrain the alteration mineralogy of ...
Ferric (Fe3+-bearing) smectites, including nontronite, constitute the majority of hydrous mineral ex...
Near-infrared remote sensing data of Mars have revealed thousands of ancient deposits of Fe/Mg-rich ...
AbstractNear-infrared remote sensing data of Mars have revealed thousands of ancient deposits of Fe/...
Aqueous alteration on Mars can produce a range of tell-tale secondary minerals [1]. Surface missions...
During its exploration of the Columbia Hills, the Mars Exploration Rover ‘‘Spirit’...
Aluminous clay deposits on Mars are recognized from remotely sensed infrared spectral features simil...
Clay minerals provide indicators of the evolution of aqueous conditions and possible habitats for li...
One of the primary science goals of Mars Science Laboratory (MSL) is to investigate layered clay min...
Clays form on Earth by near-surface weathering, precipitation in water bodies within basins, hydroth...
The search for life beyond Earth is the driving motivation for present and planned missions to Mars ...
The Noachian terrain west of the Isidis basin hosts a diverse collection of alteration minerals in r...
Clays form on Earth by near-surface weathering, precipitation in water bodies within basins, hydroth...
This dissertation is comprised of three studies investigating clay mineralogy on, or near the martia...
Seafloor hydrothermal sites generate abundant Mg- and Fe-rich clays. These clays are structurally an...
To understand the aqueous history of Mars, it is critical to constrain the alteration mineralogy of ...
Ferric (Fe3+-bearing) smectites, including nontronite, constitute the majority of hydrous mineral ex...