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MARSIS Radar Sounder Instrument

Media Photo/Video

September 25, 2017

Artists illustration
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The MARSIS radar sounder instrument on the European Space Agency’s Mars Express spacecraft is comprised of a 40 meter (about 131 feet) dipole antenna. MARSIS transmits long wavelength, low frequency radio waves that can penetrate certain geologic materials and are reflected back where the radio waves encounter a change in bulk density or composition. The radargram, a time delay rendering of the reflected radar pulses, shows a subsurface feature or reflector (upper pointing arrows) separated from the surface reflection (downward pointing arrows) in Meridiani Planum. The subsurface reflector is interpreted to be the base the Meridiani Planum deposits, about 1 kilometer (about 0.62 miles) beneath the surface.   

Image courtesy ESA/NASA/JPL/KU/Smithsonian


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    Meridiani Planum and the Search for Ice on Mars

    New findings reveal deposits on Mars that could be interpreted to be ice-rich may contain little or no ice at all, based on an analysis of radar sounder data for Meridiani Planum—an area on the planet’s equator being explored by the Opportunity rover.
    • September 25, 2017
    • News Release
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