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V. Ansan and N. Mangold 3D morphometry of valley networks on Mars from HRSC/MEX DEMs: Implications for climatic evolution through time Journal of Geophysical Research: Planets 118

Article first published online: 20 SEP 2013 | DOI: 10.1002/jgre.20117

Key Points

  • Dense valley networks have 2D and 3D geometry similar to terrestrial ones
  • Hack exponent on 13 basins show values consistent with terrestrial databases
  • Late Noachian valleys are deeper and more developed than post-Noachian valleys

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