18
views
0
recommends
+1 Recommend
0 collections
    0
    shares
      • Record: found
      • Abstract: not found
      • Article: not found

      Geochemical and mineralogical indicators for aqueous processes in the Columbia Hills of Gusev crater, Mars : AQUEOUS PROCESSES IN GUSEV CRATER, MARS

      Read this article at

      ScienceOpenPublisher
      Bookmark
          There is no author summary for this article yet. Authors can add summaries to their articles on ScienceOpen to make them more accessible to a non-specialist audience.

          Abstract

          Related collections

          Most cited references32

          • Record: found
          • Abstract: found
          • Article: not found

          In situ evidence for an ancient aqueous environment at Meridiani Planum, Mars.

          Sedimentary rocks at Eagle crater in Meridiani Planum are composed of fine-grained siliciclastic materials derived from weathering of basaltic rocks, sulfate minerals (including magnesium sulfate and jarosite) that constitute several tens of percent of the rock by weight, and hematite. Cross-stratification observed in rock outcrops indicates eolian and aqueous transport. Diagenetic features include hematite-rich concretions and crystal-mold vugs. We interpret the rocks to be a mixture of chemical and siliciclastic sediments with a complex diagenetic history. The environmental conditions that they record include episodic inundation by shallow surface water, evaporation, and desiccation. The geologic record at Meridiani Planum suggests that conditions were suitable for biological activity for a period of time in martian history.
            Bookmark
            • Record: found
            • Abstract: found
            • Article: not found

            Mars surface diversity as revealed by the OMEGA/Mars Express observations.

            The Observatoire pour la Minéralogie, l'Eau, les Glaces, et l'Activité (OMEGA) investigation, on board the European Space Agency Mars Express mission, is mapping the surface composition of Mars at a 0.3- to 5-kilometer resolution by means of visible-near-infrared hyperspectral reflectance imagery. The data acquired during the first 9 months of the mission already reveal a diverse and complex surface mineralogy, offering key insights into the evolution of Mars. OMEGA has identified and mapped mafic iron-bearing silicates of both the northern and southern crust, localized concentrations of hydrated phyllosilicates and sulfates but no carbonates, and ices and frosts with a water-ice composition of the north polar perennial cap, as for the south cap, covered by a thin carbon dioxide-ice veneer.
              Bookmark
              • Record: found
              • Abstract: not found
              • Article: not found

              Martian cratering 8: Isochron refinement and the chronology of Mars

                Bookmark

                Author and article information

                Journal
                Journal of Geophysical Research: Planets
                J. Geophys. Res.
                American Geophysical Union (AGU)
                01480227
                February 2006
                February 2006
                : 111
                : E2
                : n/a
                Article
                10.1029/2005JE002560
                525f2a1c-e0e6-454d-a75e-4903520e5542
                © 2006

                http://doi.wiley.com/10.1002/tdm_license_1.1

                History

                Comments

                Comment on this article