Eroded Ejecta
About this image
The ejecta material of the impact crater observed in this THEMIS image is partly eroded as the trend of a regional geologic unit is beginning to emerge from beneath the blanket. The aligned texture is caused by wind erosion which formed yardangs.
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
Context
Image ID:
V05810009 (View data in Mars Image Explorer)
8.7784
202.458
5810
2003-04-06 14:19
Thu, 2003-05-01
VIS
1024 pixels (18 km)
3648 pixels (65 km)
0.017926 km/pixel
0.018056 km/pixel