Literature DB >> 20950170

The Mawrth Vallis region of Mars: A potential landing site for the Mars Science Laboratory (MSL) mission.

Joseph R Michalski1, François Poulet, Damien Loizeau, Nicolas Mangold, Eldar Noe Dobrea, Janice L Bishop, James J Wray, Nancy K McKeown, Mario Parente, Ernst Hauber, Francesca Altieri, F Giacomo Carrozzo, Paul B Niles.   

Abstract

The primary objective of NASA's Mars Science Laboratory (MSL) mission, which will launch in 2011, is to characterize the habitability of a site on Mars through detailed analyses of the composition and geological context of surface materials. Within the framework of established mission goals, we have evaluated the value of a possible landing site in the Mawrth Vallis region of Mars that is targeted directly on some of the most geologically and astrobiologically enticing materials in the Solar System. The area around Mawrth Vallis contains a vast (>1 × 10⁶ km²) deposit of phyllosilicate-rich, ancient, layered rocks. A thick (>150 m) stratigraphic section that exhibits spectral evidence for nontronite, montmorillonite, amorphous silica, kaolinite, saponite, other smectite clay minerals, ferrous mica, and sulfate minerals indicates a rich geological history that may have included multiple aqueous environments. Because phyllosilicates are strong indicators of ancient aqueous activity, and the preservation potential of biosignatures within sedimentary clay deposits is high, martian phyllosilicate deposits are desirable astrobiological targets. The proposed MSL landing site at Mawrth Vallis is located directly on the largest and most phyllosilicate-rich deposit on Mars and is therefore an excellent place to explore for evidence of life or habitability.

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Year:  2010        PMID: 20950170     DOI: 10.1089/ast.2010.0491

Source DB:  PubMed          Journal:  Astrobiology        ISSN: 1557-8070            Impact factor:   4.335


  4 in total

Review 1.  Subsurface water and clay mineral formation during the early history of Mars.

Authors:  Bethany L Ehlmann; John F Mustard; Scott L Murchie; Jean-Pierre Bibring; Alain Meunier; Abigail A Fraeman; Yves Langevin
Journal:  Nature       Date:  2011-11-02       Impact factor: 49.962

2.  Remote Detection of Clay Minerals.

Authors:  Janice L Bishop; Joseph R Michalski; John Carter
Journal:  Dev Clay Sci       Date:  2017-10-13

3.  Multiple mineral horizons in layered outcrops at Mawrth Vallis, Mars, signify changing geochemical environments on early Mars.

Authors:  Janice L Bishop; Christoph Gross; Jacob Danielsen; Mario Parente; Scott L Murchie; Briony Horgan; James J Wray; Christina Viviano; Frank P Seelos
Journal:  Icarus       Date:  2020-01-17       Impact factor: 3.508

4.  Discovery of recurring slope lineae candidates in Mawrth Vallis, Mars.

Authors:  Anshuman Bhardwaj; Lydia Sam; F Javier Martín-Torres; María-Paz Zorzano
Journal:  Sci Rep       Date:  2019-02-14       Impact factor: 4.379

  4 in total

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