The Noachian terrain west of the Isidis basin hosts a diverse collection of alteration minerals
in rocks comprising varied geomorphic units within a 100,000 km2 region in and near the …

Martian aqueous mineral deposits have been examined and characterized using data
acquired during Mars Reconnaissance Orbiter's (MRO) primary science phase, including …

Analysis of visible to near infrared reflectance data from the MRO CRISM hyperspectral
imager has revealed the presence of an ovoid-shaped landform, approximately 3 by 5km in …

Columbus crater in the Terra Sirenum region of the Martian southern highlands contains
light‐toned layered deposits with interbedded sulfate and phyllosilicate minerals, a rare …

Juventae Chasma contains four light‐toned sulfate‐bearing mounds (denoted here as A–D
from west to east) inside the trough, mafic outcrops at the base of the mounds and in the wall …

The region surrounding the Mawrth Vallis outflow channel on Mars hosts thick layered
deposits containing diverse phyllosilicate minerals. Here we report detection of the Ca …

High-resolution spectral images reveal many new exposures of hydrated minerals across
the Noachian southern highlands of Mars. Several different phyllosilicates are observed …

Phyllosilicate deposits on Mars provide an opportunity to evaluate aqueous activity and the
possibility that habitable environments may have existed during the Noachian period there …

Analyses of MRO/CRISM images of the greater Mawrth Vallis region of Mars affirm the
presence of two primary phyllosilicate assemblages throughout a region∼ 1000× 1000 km …

Mawrth Vallis contains one of the largest exposures of phyllosilicates on Mars. Nontronite,
montmorillonite, kaolinite, and hydrated silica have been identified throughout the region …