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  2. Mars Orbiter Laser Altimeter - Wikipedia

    en.wikipedia.org/wiki/Mars_Orbiter_Laser_Altimeter

    A laser altimeter is an instrument that measures the distance from an orbiting spacecraft to the surface of the planet or asteroid that the spacecraft is orbiting. The distance is determined by measuring the complete round trip time of a laser pulse from the instrument to the body's surface, and back to the instrument.

  3. Ismenius Lacus quadrangle - Wikipedia

    en.wikipedia.org/wiki/Ismenius_Lacus_quadrangle

    Interactive image map of the global topography of Mars. Hover your mouse over the image to see the names of over 60 prominent geographic features, and click to link to them. Coloring of the base map indicates relative elevations, based on data from the Mars Orbiter Laser Altimeter on NASA's Mars Global Surveyor.

  4. Geology of Mars - Wikipedia

    en.wikipedia.org/wiki/Geology_of_Mars

    Mars Orbital Laser Altimeter (MOLA) colorized shaded-relief maps showing elevations in the western and eastern hemispheres of Mars. (Left): The western hemisphere is dominated by the Tharsis region (red and brown). Tall volcanoes appear white. Valles Marineris (blue) is the long gash-like feature to the right.

  5. LANL-developed instrument fires data-collecting laser on Mars ...

    www.aol.com/lanl-developed-instrument-fires-data...

    The instrument "zaps" rocks on Mars's surface with a laser and collects the light created by the resulting plasma. That light is then analyzed to determine the present elements.

  6. Mars Global Surveyor - Wikipedia

    en.wikipedia.org/wiki/Mars_Global_Surveyor

    It operated as an altimeter until a portion of the laser reached end-of-life in June 2001. The instrument then functioned as a radiometer until October 2006. [12] High resolution topographic map of Mars based on the Mars Global Surveyor laser altimeter research led by Maria Zuber and David Smith. North is at the top.

  7. Thaumasia quadrangle - Wikipedia

    en.wikipedia.org/wiki/Thaumasia_quadrangle

    These networks are evidence that Mars may have once been warmer, wetter, and perhaps had precipitation in the form of rain or snow. A study with the Mars Orbiter Laser Altimeter, Thermal Emission Imaging System (THEMIS) and the Mars Orbiter Camera (MOC) support the idea that Warrego Valles was formed from precipitation. [31]

  8. Aeolis quadrangle - Wikipedia

    en.wikipedia.org/wiki/Aeolis_quadrangle

    Coloring of the base map indicates relative elevations, based on data from the Mars Orbiter Laser Altimeter on NASA's Mars Global Surveyor. Whites and browns indicate the highest elevations (+12 to +8 km); followed by pinks and reds (+8 to +3 km); yellow is 0 km; greens and blues are lower elevations (down to −8 km).

  9. Eridania quadrangle - Wikipedia

    en.wikipedia.org/wiki/Eridania_quadrangle

    Coloring of the base map indicates relative elevations, based on data from the Mars Orbiter Laser Altimeter on NASA's Mars Global Surveyor. Whites and browns indicate the highest elevations (+12 to +8 km); followed by pinks and reds (+8 to +3 km); yellow is 0 km; greens and blues are lower elevations (down to −8 km).