Figure 6: THEMIS VIS image V03810003, showing the westernmost flat-topped area of the massif in Coprates Chasma and a dark, competent layer below the level of the flat top. This layer can clearly be seen, even on sunward-facing slopes, demonstrating that it has a lower albedo. This dark layer is indicated by arrows.
Return to Layering stratigraphy of eastern Coprates and northern Capri Chasmata, Mars.
A version of this figure was published by Elsevier Inc. Copyright © 2005 Ross A. Beyer.