Lava Flows of Daedalia Planum

Scaled Image

Image Credit: NASA/JPL/ASU

About this image

This THEMIS image captures a portion of several lava flows in Daedalia Planum southwest of the Arsia Mons shield volcano. Textures characteristic of the variable surface roughness associated with different lava flows in this region are easily seen. The lobate edges of the flows are distinctive, and permit the discrimination of many over-lapping individual flows. The surfaces of some flows look wrinkly and ropy, probably indicating a relatively fluid type of lava flow referred to as pahoehoe. The surface textures of lava flows can thus sometimes be used for comparative purposes to infer lava viscosity and effusion rates. Numerous parallel curved ridges are visible on the upper surfaces of some of the lava flows. These ridges make the flow surface look somewhat ropy, and at smaller scales this flow might be referred to as pahoehoe, however, these features are probably better referred to as pressure ridges. Pressure ridges form on the surface of a lava flow when the upper part of the flow is exposed to air, cooling it, but the insulated much warmer interior of the flow continues to move down slope (and more material is pushed forward from behind), causing the surface to compress and pile up like a rug.

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


Image ID: 
V01578003 (View data in Mars Image Explorer)
2002-04-23 03:52
Mon, 2002-10-21
1024 pixels (17 km)
3648 pixels (62 km)
0.017103 km/pixel
0.017228 km/pixel


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