The Mars Science Laboratory (MSL) rover will land in Gale Crater on Mars in August 2012. The planned landing site is an alluvial fan near the base of the crater's central mound. Orbital remote sensing of this 5 km high mound indicates the presence of hydrated sulfates, interstratified with smectite and hematite-bearing layers. Minerals formed in an aqueous environment are of particular interest given that water is a fundamental ingredient of living systems and that MSL's prime science objective is to investigate martian habitability.


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    Titel :

    Definitive Mineralogy from the Mars Science Laboratory Chemin Instrument


    Beteiligte:
    Yen, A. S. (Autor:in) / Bish, D. L. (Autor:in) / Blake, D. F. (Autor:in) / Vaniman, D. T. (Autor:in) / Treiman, A. H. (Autor:in) / Ming, D. W. (Autor:in) / Morris, Richard V. (Autor:in) / Farmer, J. D. (Autor:in) / Downs, R. T. (Autor:in) / Chipera, S. J. (Autor:in)

    Kongress:

    43rd Lunar and Planetary Science Conference ; 2012 ; The Woodlands, TX, United States


    Erscheinungsdatum :

    2012-01-01


    Medientyp :

    Aufsatz (Konferenz)


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :