[1] The Nili Fossae region located on the northwestern quadrant of the Isidis Basin, Mars, displays superb exposures of bedrock outcrops that reveal mineralogy and composition of the crust. Previous work has shown that this region exhibits the largest exposures of olivine-dominated rock units on Mars. Visible-infrared imaging spectrometer data acquired by OMEGA were calibrated to surface reflectance and analyzed to determine surface mineralogy. The dominant minerals identified are iron-bearing mafic silicates (low- and high-calcium pyroxene, olivine) and water-bearing phyllosilicate (iron-rich smectite clay). The strength and position of mineral absorption features were used to produce mineral indicator maps for the dominant species, and th...
The Noachian terrain west of the Isidis basin hosts a diverse collection of alteration minerals in r...
[1] The igneous evolution of Mars is well represented in stratigraphic settings that transition acro...
Phyllosilicates, a class of hydrous mineral first definitively identified on Mars by the OMEGA (Obse...
Nili Fossaeis a region with fresh exposures of old material. OMEGA spectral data have revealed a str...
We have detected a 30,000-square-kilometer area rich in olivine in the Nili Fossae region of Mars. N...
Context. Phyllosilicates were definitely identified on Mars by the OMEGA (Observatoire pour la Minér...
There is ample evidence of ancient and long-lasting fluvial activity and chemical alteration in the ...
l’Activite ́ (OMEGA) imaging spectrometer on board Mars Express has acquired data coverage of the Ma...
The identification and classification of minerals on the Martian surface can provide important infor...
Oxia Planum is a Noachian plain on Mars. It was chosen as the final landing site for in situ studies...
[1] Definitive exposures of pristine, ancient crust on Mars are rare, and the finding that much of t...
International audienceThe European Space Agency and Roscosmos' ExoMars rover mission, which is plann...
The enhanced spatial and spectral resolution provided by the Compact Reconnaissance Imaging Spectrom...
The enhanced spatial and spectral resolution provided by the Compact Reconnaissance Imaging Spectrom...
The Noachian terrain west of the Isidis basin hosts a diverse collection of alteration minerals in r...
[1] The igneous evolution of Mars is well represented in stratigraphic settings that transition acro...
Phyllosilicates, a class of hydrous mineral first definitively identified on Mars by the OMEGA (Obse...
Nili Fossaeis a region with fresh exposures of old material. OMEGA spectral data have revealed a str...
We have detected a 30,000-square-kilometer area rich in olivine in the Nili Fossae region of Mars. N...
Context. Phyllosilicates were definitely identified on Mars by the OMEGA (Observatoire pour la Minér...
There is ample evidence of ancient and long-lasting fluvial activity and chemical alteration in the ...
l’Activite ́ (OMEGA) imaging spectrometer on board Mars Express has acquired data coverage of the Ma...
The identification and classification of minerals on the Martian surface can provide important infor...
Oxia Planum is a Noachian plain on Mars. It was chosen as the final landing site for in situ studies...
[1] Definitive exposures of pristine, ancient crust on Mars are rare, and the finding that much of t...
International audienceThe European Space Agency and Roscosmos' ExoMars rover mission, which is plann...
The enhanced spatial and spectral resolution provided by the Compact Reconnaissance Imaging Spectrom...
The enhanced spatial and spectral resolution provided by the Compact Reconnaissance Imaging Spectrom...
The Noachian terrain west of the Isidis basin hosts a diverse collection of alteration minerals in r...
[1] The igneous evolution of Mars is well represented in stratigraphic settings that transition acro...
Phyllosilicates, a class of hydrous mineral first definitively identified on Mars by the OMEGA (Obse...