Geochemical constraints on the presence of clay minerals in the Burns formation, Meridiani Planum, Mars

@article{Cino2014GeochemicalCO,
  title={Geochemical constraints on the presence of clay minerals in the Burns formation, Meridiani Planum, Mars},
  author={C. Cino and E. Dehouck and S. McLennan},
  journal={Icarus},
  year={2014},
  volume={281},
  pages={137-150}
}
Abstract Burns formation sandstones, deposited by aeolian processes and preserved at Meridiani Planum, Mars, contain abundant sulfate minerals. These sedimentary rocks are thought to be representative of a sulfate-rich geological epoch during late Noachian – early Hesperian time that followed an earlier clay-rich epoch. Twenty Burns formation targets, abraded by the Rock Abrasion Tool (RAT) and for which alpha-particle X-ray spectrometry (APXS) and Mossbauer spectroscopy data are available… Expand

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