Scaled Image

Image Credit: NASA/JPL/ASU

About this image

Remarkable differences in brightness and texture are apparent between these lava flows found on the southern flanks of Arsia Mons. These differences could be due to variations in composition, age, vesicularity, or degrees of weathering.

Please see the THEMIS Data Citation Note for details on crediting THEMIS images. 

Context

Image ID: 
V07008001 (View data in Mars Image Explorer)
-19.5406
238.37
7008
2003-07-14 03:16
Thu, 2003-07-31
VIS
1024 pixels (17 km)
3648 pixels (62 km)
0.017249 km/pixel
0.017375 km/pixel

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