Geochemical reservoirs and timing of sulfur cycling on Mars

F Gaillard, J Michalski, G Berger, SM McLennan… - Space Science …, 2013 - Springer
Sulfate-dominated sedimentary deposits are widespread on the surface of Mars, which
contrasts with the rarity of carbonate deposits, and indicates surface waters with chemical …

Revised CRISM spectral parameters and summary products based on the currently detected mineral diversity on Mars

CE Viviano, FP Seelos, SL Murchie… - Journal of …, 2014 - Wiley Online Library
The investigation of hyperspectral data from the Mars Reconnaissance Orbiter Compact
Reconnaissance Imaging Spectrometer for Mars (CRISM) and the Observatoire pour la …

[HTML][HTML] The evidence for unusually high hydrogen abundances in the central part of Valles Marineris on Mars

I Mitrofanov, A Malakhov, M Djachkova, D Golovin… - Icarus, 2022 - Elsevier
Studies of hydrogen deposition in the shallow Martian subsurface have been conducted by
two neutron and one gamma-ray detectors in the past and provided global hydrogen maps …

Extensive surface pedogenic alteration of the Martian Noachian crust suggested by plateau phyllosilicates around Valles Marineris

L Le Deit, J Flahaut, C Quantin… - Journal of …, 2012 - Wiley Online Library
Thousands of phyllosilicate‐rich outcrops, mainly iron or magnesium‐rich are exposed on
Noachian terrains in the Martian southern highlands. We analyzed 90 CRISM observations …

One million cubic kilometers of fossil ice in Valles Marineris: Relicts of a 3.5 Gy old glacial landsystem along the Martian equator

M Gourronc, O Bourgeois, D Mège, S Pochat, B Bultel… - Geomorphology, 2014 - Elsevier
Self-consistent landform assemblages suggest that Valles Marineris, the giant valley system
that stretches along the Martian equator, was entirely glaciated during Late Noachian to …

Variability in martian sinuous ridge form: Case study of Aeolis Serpens in the Aeolis Dorsa, Mars, and insight from the Mirackina paleoriver, South Australia

RME Williams, RP Irwin III, DM Burr, T Harrison… - Icarus, 2013 - Elsevier
In the largest known population of sinuous ridges on Mars, Aeolis Serpens stands out as the
longest (∼ 500km) feature in Aeolis Dorsa. The formation of this landform, whether from …

Mixtures of clays and sulfates within deposits in western Melas Chasma, Mars

CM Weitz, EN Dobrea, JJ Wray - Icarus, 2015 - Elsevier
We have utilized several data sets from multiple spacecraft that have been acquired over a
continuous observation campaign across the southwestern Melas Chasma region of Mars …

Gypsum, opal, and fluvial channels within a trough of Noctis Labyrinthus, Mars: Implications for aqueous activity during the Late Hesperian to Amazonian

CM Weitz, JL Bishop, JA Grant - Planetary and Space Science, 2013 - Elsevier
We investigate in detail the morphology, mineralogy, and stratigraphy of light-toned deposits
within one trough of Noctis Labyrinthus, centered at− 6.8° N, 261.1° E. CRISM spectra taken …

Estimating kaolinite crystallinity using near-infrared spectroscopy: Implications for its geology on Earth and Mars

M Pineau, M Mathian, F Baron, B Rondeau… - American …, 2022 - degruyter.com
Kaolinite is an Al-rich phyllosilicate commonly observed on Earth as a product of the
chemical weathering of aluminosilicates. It has also been detected on the martian surface by …

Atmospheric origin of Martian interior layered deposits: Links to climate change and the global sulfur cycle

J Michalski, PB Niles - Geology, 2012 - pubs.geoscienceworld.org
Since the first photogeologic exploration of Mars, vast mounds of layered sediments found
within the Valles Marineris troughs (interior layered deposits, ILDs) have remained …