Points of interest:
- White splotches - alteration minerals? (Sulfates?). Clustered in top centre of image.
- Dark grey brown material: dominant material here. Doesn't appear to be the famous purple coating material. Friable (crumbly), based on the HazCam images, but seems to be more resistant/better represented than the rest of the stuff in this rock. Features fine cracks/fractures/joints. Most of it is dull, but some appears to have a bit of lustre (shiny) - see upper right.
- Light grey zones: They feature "spots" - embedded tan regions, and smaller darker regions. Some of it is covered by white splotches, but some zones have none whatsoever. See top centre for some clear examples.
- Isolated tan zones: Smaller than the light grey zones, and almost entirely free of white splotches. Clustered nicely at right centre.
- Small dark elongated clasts, light brown and black.
- Small patches of purplish material: the usual coating material? Very little of it here. See lower left.
Now in a place like this, you always have to consider an impact origin: we're on the edge of a fair-sized impact crater and we've found plenty of material that was heavily modified/created by one or more serious impacts, including three of the four samples we've actually managed to bag on the rim. Impact breccia is complex stuff, a salad of ejected material that gets fused together and then solidifies into a chaotic and beautiful mass.
In this case, however, I really have to wonder. If this is impact breccia - even a breccia altered by long-lasting groundwater - I haven't seen a texture like it. The light grey zones and tan zones have fairly round outlines, rather than angular ones, which you would expect from shards of broken and ejected material. The distribution of the different zones (tan and grey zones tend to be grouped in small areas) doesn't seem random.
All in all, for me this is one of the most fascinating images of the entire mission, and that's saying something.
😃 I hope some rover drivers get to see this question - it's a very good one, just funny if you've seen the whole mission.
In the past - before Curiosity landed - NASA definitely chose rover landing sites based in part on their (presumed) smoothness and traversability (e.g. Opportunity). This was also true for the first Chinese lander.
In the case of Perseverance, the "rockiness" in this region actually varies quite a bit over fairly short distances. The terrain we've been exploring since late 2024 was chosen for two reasons: ease of traversal (when we were climbing out of the Jezero Crater) and science (our current location, Witch Hazel Hill). When we were down on the old river delta last year, though, the rover drivers had a very difficult time with terrain like this and this.
Witch Hazel Hill is smooth in part because the bedrock here is soft and easily eroded. Quite a bit of it has significant clay content, like you'd find in Earth soils, due to heavy interaction with water in the geologic past. Down on the crater floor where we landed, where the terrain is made of volcanic rocks, there are scenes like this. In the end, the rover drivers are pretty protective of their vehicle, so we tend to prefer smooth stretches for driving.