Image Credit: NASA/JPL/ASU
|
Context image credit: NASA/JPL/MOLA
View on map Detailed information on this image is available at the
THEMIS Data Releases website.
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
Chaotic terrain, arcuate fractures and erosional remanents make up the bulk of geologic features within this Themis VIS image. The arcuate fractures and chaotic terrain could possibly have formed due to a volitile rich subsurface layer being changed by erosion/exposure causing the upper lying surface to fracture and collapse.
|
||||||||||||