Dark Light
Data from other instruments, such as THEMIS and CRISM, imply that chlorides are present here; the CRISM data reveal that iron/magnesium clays are also present.

Our goal is to compare textures and determine stratigraphy for these two materials. Enhanced color very useful for mapping units of distinct composition.


Image: NASA/JPL/University of Arizona https://www.uahirise.org/hipod/ESP_016162_1495
Related Posts

The Saga of Airy-0

Up to now, we’ve never imaged Airy-0, a crater within Airy Crater that formerly was used to define zero longitude on Mars.

Layers in a Crater

Located to the north of Cassini Crater, the objective of this observation is to confirm the presence of…
Deuteronilus Mensae

The Hanging Crater

Queen Amytis had her Hanging Gardens in Babylon, and Mars has its hanging crater! This impact crater appears…
Impact crater

Impact Craters as Windows to What Lies Beneath

Impact craters are common on all solar system bodies. They offer many clues to scientists regarding the geologic history of a planetary surface, particularly regarding its age, evolution with time, and composition.