Martian surface

Numéro d’image : 11593751
Martian surface
Martian surface. This region is on the northern edge of the Magellan Crater in the Tharsis volcanic region. At top centre are mounds of rock,measuring up to 2 kilometres tall. It is not known how these mounds were formed,but they could be due to subrosion. Subrosion occurs when volcanic activity melts frozen ground water,which erodes underground cavities as it flows away. The cavities collapse due to weight from above,leaving irregular mounds on the surface. Image taken by the High-Resolution Stereo Camera (HRSC) on the Mars Express spacecraft
Licence : Droits gérés
Crédit: Science Photo Library / Neukum, G. / FU Berlin / ESA / DLR
Taille de l’image : 5531 px × 3210 px
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Property Release : Non requis
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