File:Layers some with overhang ESP 26270 1820.jpg

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Description	Layers with some showing an overhang. Layers exposed on the sides of hills are visible as terraced steps. The formation of these steps is a result in differences between layers in cohesion and resistance to weathering. Weaker layers disaggregate quickly into shallow slopes, while stronger layers maintain steep “sharp” appearing edges. Such contrast can occur, for example, between alternating strong lava flows and weak volcanic ash deposits.
Date	November 21, 2012
Source	https://www.uahirise.org/ESP_027747_1820
Author	Jim Secosky selected pictures from NASA files. The credit should read NASA/JPL-Caltech/UArizona.

File:Layers some with overhang ESP 26270 1820.jpg

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public domain

MIME type

image/jpeg

checksum

6b8af534b59b76729d2aac1ad1b9453d79fb2e48

data size

495,201 byte

height

817 pixel

width

1,829 pixel

coordinates of the point of view

2°9'46.800"N, 9°2'20.400"W

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