This paper associates phyllosilicates with polygonal lineations in HiRise imagery, and offers some other interesting observations regarding the directions that some of the layers dip.
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3. Morphology and Stratigraphy
[10] Images of the phyllosilicate-bearing crater rim segments from the MRO High Resolution Imaging Science Experiment (HiRISE) [McEwen et al., 2007] reveal layering and a range of polygonal textures (Figure 3a), similar in appearance to other phyllosilicate-bearing outcrops in Meridiani [Wiseman et al., 2008; Marzo et al., 2009] and many other locations on Mars [e.g., Wray et al., 2008; Bishop et al., 2008; Ehlmann et al., 2009]. Stereo views (Figure 3b) show that layers within the western rim dip away from the crater interior, as expected if the beds predate Endeavour crater and were back-tilted by the impact. In contrast, bright layers bounding many Endeavour rim segments [e.g., McEwen et al., 2009, Figure 29] dip down toward the crater interior; we cannot clearly determine whether these layers predate or postdate the impact based on orbital images.