ESAESA ScienceMars Express
   
Europe goes to Mars
About Mars Express
About Mars
Meet the team
Multimedia
VideoTalkMars Express imagesMars Express videosHRSC videosAnimation in 11 languagesDownload wallpapersDownload screensavers3D Flash 'model'Make a model
Services
Comments Bookmark and Share
 
 
 
 
Article Images
Rim of Crater Huygens on Mars
 
19 October 2004

Huygens Crater Rim - 3-channels colour image
Download:
 HI-RES JPEG (Size: 1474 kb)  HI-RES TIFF (Size: 8 716kb)
This image of the eastern rim of the Martian impact crater Huygens was taken during orbit 532 on 20 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.

The crater rim is heavily eroded and shows a ‘dendritic’ pattern. This observation suggests surface water run-off.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.

Credits: ESA/DLR/FU Berlin (G. Neukum)

 
 
Huygens Crater Rim - perspective view
Download:
 HI-RES JPEG (Size: 1 560 kb)  HI-RES TIFF (Size: 8532 kb)
This perspective view of the eastern rim of the Martian impact crater Huygens was taken during orbit 532 on 20 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.

Credits: ESA/DLR/FU Berlin (G. Neukum)
 
 
Huygens Crater Rim - context image
Download:
 HI RES JPG (Size: 3853 kb)
This map shows the region displayed in the main images, the crater rim indicated here in context, centred around longitude 61° East and latitude 14° South.

Credits: ESA/DLR/FU Berlin (G. Neukum)
 
 
Huygens Crater Rim - grayscale nadir image
Download:
 HI-RES JPEG (Size: 1089 kb)  HI-RES TIFF (Size: 5740 kb)
Here part of the eastern rim of Crater Huygens is shown. The crater rim is heavily eroded and shows a ‘dendritic’ pattern. This observation suggests surface water run-off.

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.

The image was taken during orbit 532 on 20 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.

Credits: ESA/DLR/FU Berlin (G. Neukum)

 
 
Huygens Crater Rim - red-cyan anaglyph image
Download:
 HI-RES JPEG (Size: 987 kb)  HI-RES TIFF (Size: 10 655 kb)
This 3D anaglyph image shows the eastern rim of Crater Huygens. The crater rim is heavily eroded and shows clearly the ‘dendritic’ patterns of flow channels. From above, they look like a tree or a river delta in reverse. This observation suggests surface water run-off.

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.

The image was taken during orbit 532 on 20 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.

Credits: ESA/DLR/FU Berlin (G. Neukum)

 
 
Huygens Crater Rim - perspective view
Download:
 HI-RES JPEG (Size: 1398 kb)  HI-RES TIFF (Size: 7871 kb)
This perspective view of the rim of Crater Huygens was taken during orbit 532 on 20 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.

This close-up view shows the heavily eroded crater rim, and part of the basin that has been subsequently filled by sediments transported into the crater.

Credits: ESA/DLR/FU Berlin (G. Neukum)

 


Looking at Mars
Mars Express image browser
Recent images
Crater Hale in Argyre basinCoprates Catena’s ‘collapsed’ structuresMartian moon Phobos in detailTithonium Chasma, Valles Marineris, on MarsPromethei Terra, southern highlands of MarsOphir Chasma, part of Valles MarinerisSolis Planum, Thaumasia regionEos Chasma, part of Valles MarinerisCrater dunes in Argyre PlanitiaThe eroded valleys of Dao and Niger VallesOlympus Mons caldera in perspectiveEscarpment and landslides of Olympus MonsView of deposits in Melas Chasma on Mars
More information
High Resolution Stereo CameraBehind the lens...
 
 
 
   Copyright 2000 - 2010 © European Space Agency. All rights reserved.