scispace - formally typeset
Journal ArticleDOI

Hydrated silicate minerals on Mars observed by the Mars Reconnaissance Orbiter CRISM instrument

Reads0
Chats0
TLDR
The diversity of phyllosilicate mineralogy is expanded with the identification of kaolinite, chlorite and illite or muscovite, and a new class of hydrated silicate (hydrated silica).
Abstract
Phyllosilicates, a class of hydrous mineral first definitively identified on Mars by the OMEGA (Observatoire pour la Mineralogie, L'Eau, les Glaces et l'Activitie) instrument, preserve a record of the interaction of water with rocks on Mars. Global mapping showed that phyllosilicates are widespread but are apparently restricted to ancient terrains and a relatively narrow range of mineralogy (Fe/Mg and Al smectite clays). This was interpreted to indicate that phyllosilicate formation occurred during the Noachian (the earliest geological era of Mars), and that the conditions necessary for phyllosilicate formation (moderate to high pH and high water activity) were specific to surface environments during the earliest era of Mars's history. Here we report results from the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) of phyllosilicate-rich regions. We expand the diversity of phyllosilicate mineralogy with the identification of kaolinite, chlorite and illite or muscovite, and a new class of hydrated silicate (hydrated silica). We observe diverse Fe/Mg-OH phyllosilicates and find that smectites such as nontronite and saponite are the most common, but chlorites are also present in some locations. Stratigraphic relationships in the Nili Fossae region show olivine-rich materials overlying phyllosilicate-bearing units, indicating the cessation of aqueous alteration before emplacement of the olivine-bearing unit. Hundreds of detections of Fe/Mg phyllosilicate in rims, ejecta and central peaks of craters in the southern highland Noachian cratered terrain indicate excavation of altered crust from depth. We also find phyllosilicate in sedimentary deposits clearly laid by water. These results point to a rich diversity of Noachian environments conducive to habitability.

read more

Citations
More filters
Journal ArticleDOI

Multi- and hyperspectral geologic remote sensing: A review

TL;DR: A review of multispectral and hyperspectral remote sensing data, products and applications in geology shows a unique opportunity to develop standardized protocols leading to validated and reproducible products from satellite remote sensing for the geology community.

Multi - and hyperspectral geologic remote sensing : a review

TL;DR: A review of multispectral and hyperspectral remote sensing data, products and applications in geology can be found in this paper, where the authors provide an overview of the main threats for geologic remote sensing lies in the lack of data continuity.
Journal ArticleDOI

Subsurface water and clay mineral formation during the early history of Mars

TL;DR: Clay minerals, recently discovered to be widespread in Mars’s Noachian terrains, indicate long-duration interaction between water and rock over 3.7 billion years ago, and available data indicate substantial Martian clay formation by hydrothermal groundwater circulation and a Noachia rock record dominated by evidence of subsurface waters.
References
More filters
Journal ArticleDOI

High spectral resolution reflectance spectroscopy of minerals

TL;DR: In this article, the reflectance spectra of minerals are studied as a function of spectral resolution in the range from 0.2 to 3.0 microns, and selected absorption bands were studied at resolving powers as high as 2240.
Journal ArticleDOI

Context Camera Investigation on board the Mars Reconnaissance Orbiter

TL;DR: The Context Camera (CTX) on the Mars Reconnaissance Orbiter (MRO) is a Facility Instrument (i.e., government-furnished equipment operated by a science team not responsible for design and fabrication) designed, built, and operated by Malin Space Science Systems and the MRO Mars Color Imager team (MARCI) as mentioned in this paper.
Related Papers (5)