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  2. Areography - Wikipedia

    en.wikipedia.org/wiki/Areography

    On Earth, the zero elevation datum is based on sea level (the geoid). Since Mars has no oceans and hence no 'sea level', it is convenient to define an arbitrary zero-elevation level or "vertical datum" for mapping the surface, called areoid. [9] The datum for Mars was defined initially in terms of a constant atmospheric pressure.

  3. Airy-0 - Wikipedia

    en.wikipedia.org/wiki/Airy-0

    Airy-0 is a crater inside the larger Airy Crater on Mars, whose location historically defined the Martian prime meridian.It is about 0.5 km (0.3 mile) across and lies within the dark region Sinus Meridiani, one of the early albedo features to be identified on Mars.

  4. List of mountains on Mars - Wikipedia

    en.wikipedia.org/wiki/List_of_mountains_on_Mars

    Listed are the elevations of the peaks (the vertical position relative to the areoid, which is the Martian vertical datum — the surface defined as zero elevation by average martian atmospheric pressure and planet radius), which is not the height above the surrounding terrain (topographic prominence). Listed mons elevation is the highest point ...

  5. New 3-D map of Mars' ice caps reveal hidden structures - AOL

    www.aol.com/news/2017-01-05-new-3-d-map-of-mars...

    Scientists have announced the discovery of structures like layering and potential impact craters which had been hidden under Mars’ polar ice caps. New 3-D map of Mars' ice caps reveal hidden ...

  6. Vertical datum - Wikipedia

    en.wikipedia.org/wiki/Vertical_datum

    In some situations sea level does not apply at all – for instance for mapping Mars' surface – forcing the use of a different "zero elevation", such as mean radius. A geodetic vertical datum takes some specific zero point, and computes elevations based on the geodetic model being used, without further reference to sea levels.

  7. Jezero (crater) - Wikipedia

    en.wikipedia.org/wiki/Jezero_(crater)

    Jezero on the edge of the Isidis basin. Jezero [a] (ICAO: JZRO) is a crater on Mars in the Syrtis Major quadrangle, [3] about 45.0 km (28.0 mi) in diameter. Thought to have once been flooded with water, the crater contains a fan-delta deposit rich in clays. [4]

  8. Acidalia Planitia - Wikipedia

    en.wikipedia.org/wiki/Acidalia_Planitia

    On Mars, mud volcanoes have an average diameter of ~1 km and a relief of 10 to 180 meters. Their higher albedo is a result of more crystalline iron oxides than the rest of Acidalia Planitia. [ 8 ] Mud volcanoes erupt sediments from deep beneath the surface and change the rising rocks very minimally.

  9. File : Mars topography (MOLA dataset) with poles HiRes.jpg

    en.wikipedia.org/wiki/File:Mars_topography_(MOLA...

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