This study focused on obtaining size frequency distributions of pristine crater populations from various terrains of Mars. Images from the Viking Orbiter (VO), Mars Orbital Camera (MOC), and Thermal Emission Imaging System (THEMIS) were utilized for this study. The results may aid in providing information about crater production functions and resurfacing events on Mars.


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    Title :

    Pristine Impact Crater Populations of Mars


    Contributors:


    Publication date :

    2003-01-01


    Type of media :

    Conference paper


    Type of material :

    No indication


    Language :

    English





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