Formation of the hematite-bearing unit in Meridiani Planum: Evidence for deposition in standing water

@article{Christensen2004FormationOT,
  title={Formation of the hematite-bearing unit in Meridiani Planum: Evidence for deposition in standing water},
  author={P. Christensen and S. Ruff},
  journal={Journal of Geophysical Research},
  year={2004},
  volume={109}
}
[1] The most plausible models for the origin and evolution of a unique geologic unit in Meridiani Planum, Mars, are low-temperature precipitation of Fe oxides/oxyhydroxides from standing water, precipitation from circulating fluids of hydrothermal origin, or the thermal oxidation of magnetite-rich ash. Analysis of Odyssey Thermal Emission Imaging System (THEMIS) infrared and visible images, together with MGS TES, MOLA, and MOC data, has provided additional insight into the Meridiani region. The… Expand
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TLDR
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