• → European Space Agency

      • Space for Europe
      • Space News
      • Space in Images
      • Space in Videos
    • About Us

      • Welcome to ESA
      • DG's News and Views
      • For Member State Delegations
      • Business with ESA
      • ESA Exhibitions
      • ESA Publications
      • Careers at ESA
    • Our Activities

      • Space News
      • Observing the Earth
      • Human Spaceflight
      • Launchers
      • Navigation
      • Space Science
      • Space Engineering
      • Operations
      • Technology
      • Telecommunications & Integrated Applications
    • For Public

    • For Media

      • Media
      • ESA TV
      • Videos for professionals
      • Photos
    • For Educators

    • For Kids

    • ESA

    • Space in Images

    ESA > Space in Images > 2009 > 07 > Ma'adim Vallis context map

    Free Search (11124 images)

    Ma'adim Vallis context map

    (711.69 kB)

    (3.32 MB)

    Views: 76
    Rating: 0.00/5 (0 votes cast)

    Rate this Image

    • Currently 0 out of 5 Stars.
    • 1
    • 2
    • 3
    • 4
    • 5

    Thank you for rating!

    You have already rated this page, you can only rate it once!

    Your rating has been changed, thanks for rating!

    Share this Image

    Post to Facebook Post to MySpace Post to Delicious Post to Digg Post to Twitter

    Details

    Open/Close
    • Title Ma'adim Vallis context map
    • Released 24/07/2009 2:37 pm
    • Copyright FU Berlin/ MOLA
    • Description

      Mars Express image of a region close to Ma’adim Vallis, one of the largest canyons on Mars. After Valles Marineris, Ma’adim Vallis is one of the largest canyons on Mars. The imaged region lies south-east of Ma’adim Vallis; the pictures are centred at about 29°S and 182°E and have a ground resolution of 15 m/pixel.

      Ma’adim Vallis is located between the volcanic region of Tharsis, which harbours four volcanoes, including the largest in the Solar System, and the Hellas Planitia impact basin. The canyon, 20 km wide and 2 km deep, originates in the southern highlands close to the ‘dichotomy boundary’ and ends in Gusev crater. The dichotomy boundary is a narrow region separating the cratered highlands, located mostly in the southern hemisphere of Mars, from the northern hemisphere's lowland plains.


    TAGS

    Open/Close
    • Click on the tags to find the matching images.
    • Activity Space Science
    • Mission Mars Express

    TAGS

    Open/Close

    Details

    Open/Close

    RELATED IMAGES

    • Close to Ma'adim Vallis, nadir view
      Close to Ma'adim Vallis, nadir view
      Released: 24/07/2009
      Rating
    • Close to Ma'adim Vallis, annotated nadir view
      Close to Ma'adim Vallis, annotated nadir view
      Released: 24/07/2009
      Rating

    Connect with us

    • RSS
    • Youtube
    • Twitter
    • Flickr
    • Google Buzz
    • Facebook
    • Livestream
    • Subscribe
    • App Store
    • LATEST ARTICLES
    • · Earth Explorers take centre stag…
    • · The fast winds of Venus are gett…
    • · ExoMars 2016 set to complete con…
    • · Herschel ends operations as orbi…
    • · Europe’s space hub to open its d…
    • FAQ

    • Jobs at ESA

    • Site Map

    • Contacts

    • Terms and conditions