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Patrick Thollot, Nicolas Mangold, Véronique Ansan, Stéphane Le Mouélic, Ralph E. Milliken, Janice L. Bishop, Catherine M. Weitz, Leah H. Roach, John F. Mustard and Scott L. Murchie Most Mars minerals in a nutshell: Various alteration phases formed in a single environment in Noctis Labyrinthus Journal of Geophysical Research: Planets (1991–2012) 117

Version of Record online: 21 APR 2012 | DOI: 10.1029/2011JE004028

Key Points

  • A complex assemblage of clays, sulfates and silica found in Noctis Labyrinthus
  • Hydrothermalism and various water/rock and pH can account for mineral diversity
  • Hydrated minerals on Mars can form locally during globally cold periods

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