Rim of Crater Huygens on Mars


Huygens Crater Rim - 3-channels colour image
 
Colour view of Huygens crater rim
 
19 October 2004
 
These images, taken by the High Resolution Stereo Camera (HRSC) on board ESA’s Mars Express spacecraft, show the eastern rim of the Martian impact crater Huygens.
 
 
 
Huygens Crater Rim - perspective view
 
Rim of Crater Huygens, perspective view
 
The images were taken during orbit 532 in June 2004 with a ground resolution of approximately 70 metres per pixel. The displayed region is centred around longitude 61° East and latitude 14° South.
 
 
Huygens Crater Rim - context image
   
Map showing Huygens crater rim in context
 
Huygens is an impact structure, about 450 kilometres wide, located in the heavily cratered southern highlands of Mars. Crater counts of the rim unit of the impact basin indicate that it is almost 4000 million years old.

This implies that this basin was formed in the early history of the planet and indicates a period of heavy bombardment in roughly the first 500 million years of the planet’s lifetime.
 
 
Huygens Crater Rim - grayscale nadir image
 
Black and white view of Huygens crater rim
 
 
The basin shows an inner ring that has been subsequently filled by sediments transported into the crater.

These images show part of the eastern rim of the crater. The rim is heavily eroded and shows a ‘dendritic’ pattern. This observation suggests surface water run-off.

Dendritic systems are the most common form of drainage system found on Earth. They consist of a main ‘river’ valley with tributaries with their own tributaries. From above, they look like a tree or a river delta in reverse.
 
 
Huygens Crater Rim - red-cyan anaglyph image
 
3D image of rim of Crater Huygens
 
The valley system is blanketed by dark material, which was either transported by a fluid running through the channels or by wind-driven (‘aeolian’) processes. Part of the area has been covered by slightly redder material, which implies a different chemical composition.
 
 
Huygens Crater Rim - perspective view
 
Perspective view of rim of Crater Huygens, looking north
 
 
Image resolution has been decreased for use on the internet. The colour images were processed using the nadir (vertical view) and colour channels.

The perspective views were calculated from the digital terrain model derived from the stereo channels.

The 3D anaglyph image was created from the nadir channel and one of the stereo channels. Stereoscopic glasses are needed to view the 3D image.

For more information on Mars Express HRSC images, you might like to read our updated 'Frequently Asked Questions'.
 
 


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