Mathematics – Logic
Scientific paper
Aug 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jgre..11208s04m&link_type=abstract
Journal of Geophysical Research, Volume 112, Issue E8, CiteID E08S04
Mathematics
Logic
40
Planetary Sciences: Solar System Objects: Mars, Planetary Sciences: Solid Surface Planets: Hydrology And Fluvial Processes, Planetary Sciences: Solid Surface Planets: Erosion And Weathering, Planetary Sciences: Solid Surface Planets: Composition (1060, 3672), Planetary Sciences: Solid Surface Planets: Surface Materials And Properties
Scientific paper
Nili Fossae is a region with fresh exposures of old material. OMEGA spectral data have revealed a strong diversity of minerals in the Nili Fossae region, including mafic minerals and phyllosilicates. Phyllosilicates are found to be primarily Fe-rich smectites (a type of clay minerals). These phyllosilicates are observed only on the Noachian crust, in four types of locations: Three are without any signatures other than phyllosilicates, on (1) smooth layered deposits, (2) massive exhumed material, and (3) crater ejecta, and one type of location is associated with olivine (4) over an altered mafic unit. This diversity suggests a widespread liquid water activity and a variety of alteration processes. The formation of phyllosilicates underwent considerable reduction, if not cessation, by the time of formation of Syrtis Major lava flows in the Hesperian period. Phyllosilicates are spatially and chronologically disconnected from the fluvial and depositional landforms observed in the Nili Fossae region. Observations suggest that these landforms formed after the extensive formation of phyllosilicates during short periods of time and/or temperatures close to freezing.
Ansan Véronique
Bibring Jean-Pierre
Fassett Caleb
Gerhard Neukum
Gondet Brigitte
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