Flows from Olympus Mons
About this image
This image was collected June 2, 2002 during early northern spring. The relative timing of volcanic flows from Olympus Mons and the formation of the structural feature can be deduced by which flows are cut by the fracture and which flows fill and cross the fracture.
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
Context
Image ID:
V02064003 (View data in Mars Image Explorer)
19.8492
233.018
2064
2002-06-02 05:46
Mon, 2004-04-05
VIS
1024 pixels (18 km)
3648 pixels (66 km)
0.018283 km/pixel
0.018416 km/pixel