• → 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

    • ESA Science

    • Mars Express

    • Europe goes to Mars

      • Europe reclaims a stake in Mars exploration
      • Space age transforms our knowledge about Mars
    • About Mars Express

      • Mars Express mission facts
      • Mars Express instruments
      • The mission
      • The spacecraft
      • The launcher
    • About Mars

      • Geography of Mars
      • Water on early Mars?
      • Signatures of life
      • Facts about Mars
    • Meet the team

      • International collaboration
      • Project Manager
      • Project Scientist
      • Mars Lead Scientist
      • Principal Investigators
      • Operations
      • Industry
    • Multimedia
    • VideoTalk
    • Mars Express images
    • Mars Express videos
    • HRSC videos
    • Animation in 11 languages
    • Download wallpapers
    • Download screensavers
    • 3D Flash 'model'
    • Make a model
    • Services
    • Comments

    ESA > Our Activities > Space Science > Mars Express

    Aram Chaos in false colour

    Heavily eroded Aram Chaos

    30 May 2006

    These images, taken by the High Resolution Stereo Camera (HRSC) on board ESA's Mars Express spacecraft, show Aram Chaos, 280-km-wide circular structure characterized by chaotic terrain.

    Context map, Aram Chaos
    Map showing Aram Chaos in context

    The HRSC obtained these images during orbit 945 with a ground resolution of approximately 14 metres per pixel. The images show the region of Aram Chaos, at approximately 2° North and 340° East.

    Aram Chaos is a 280-km-wide almost-circular structure located between the outflow channel Ares Vallis and Aureum Chaos. It is one of many regions located east of Valles Marineris and characterized by chaotic terrain.


    Aram Chaos in colour
    Aram Chaos (north to the right)

    As the name 'chaos' suggests, this terrain comprises large-scale remnant massifs, large relief masses that have been moved and weathered as a block. These are heavily eroded and dominate the circular morphology, or structure, which may have formed during an impact. As seen in the colour image, these remnant massifs range from a few kilometres to approximately ten kilometres wide and have a relative elevation of roughly 1000 metres.

    Aram Chaos, black and white

    The western region of the colour image is characterized by brighter material, which seems to be layered and could be the result of sedimentary deposition. Distinct layering, causing a terrace-like appearance, is also visible east of this brighter material and in the relatively flat region located in the northwest of the colour image.

    Perspective of Aram Chaos
    Aram Chaos, perspective view

    Some scientists believe that the numerous chaotic regions located in the eastern part of Valles Marineris were the source of water or ice thought to have created the valleys that extend into Chryse Planitia. These regions are particularly interesting because they may yield clues to the relationship between Valles Marineris, the chaotic terrain, the valleys and the Chryse basin.

    Aram chaos, in 3D
    Aram Chaos, 3D anaglyph

    The colour scenes have been derived from the three HRSC-colour channels and the nadir channel. The perspective view has been calculated from the digital terrain model derived from the stereo channels. The anaglyph image was calculated from the nadir and one stereo channel. Image resolution has been decreased for use on the internet.

    For more information on Mars Express HRSC images, please read our updated FAQ (frequently asked questions).

    Rate this

    Views

    Share

    • Currently 5 out of 5 Stars.
    • 1
    • 2
    • 3
    • 4
    • 5
    Rating: 5/5 (1 votes cast)

    Thank you for rating!

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

    Your rating has been changed, thanks for rating!

    182
    Tweet
    • Mars Express image browser
    • Recent images
      • Lava tubes on Pavonis Mons
        • Extensional tectonics in Tempe Terra
          • Nanedi Valles system on Mars
            • 'Happy face' crater on Mars
              • The Libya Montes valley on Mars
                • 'Hourglass'-shaped crater - new video and perspectives
                  • Eastern scarp of Olympus Mons
                    • Ausonia Mensa remnant massif
                      • Pits and tectonic grabens in Phlegethon Catena
                        • Claritas Fossae region of Mars
                          • Sulphate deposits in Juventae Chasma
                            • ‘Butterfly’ impact crater in Hesperia Planum
                              • Fly over the Chasma Boreale at Martian north pole
                                • The Biblis Patera volcano
                                • High Resolution Stereo Camera
                                  • Behind the lens...

    Connect with us

    • RSS
    • Youtube
    • Twitter
    • Flickr
    • G+
    • Facebook
    • Livestream
    • Subscribe
    • App Store
    • LATEST ARTICLES
    • · Rare merger reveals secrets of gal…
    • · Watching for hazards: ESA opens as…
    • · ESA astronaut Timothy Peake set fo…
    • · Space drives e-mobility
    • · Proba-V opens its eyes
    • FAQ

    • Jobs at ESA

    • Site Map

    • Contacts

    • Terms and conditions