Sol 1361: WATSON Camera (Raw colour) acquired on Dec. 18, 2024 at the local mean solar time of 12:42:15.
Interestingly the patch shows no tool marks from the abrasion bit
Image Credit: NASA/JPL-Caltech
Sol 1361: WATSON Camera (Raw colour) acquired on Dec. 18, 2024 at the local mean solar time of 12:42:15.
Interestingly the patch shows no tool marks from the abrasion bit
Image Credit: NASA/JPL-Caltech
A great deal.
The above is not a complete list. The dust and weathering rinds Paul Hammond mentions (the undisturbed outer surface of the rock), in general, prevent you from answering these questions in the same detail, or at all. By answering the first two questions above, you get a good idea of how the rock formed and what it contains (e.g. is this volcanic rock - like from a lava flow - or something laid down in calm water, or something else entirely)?
Generally speaking, if the mission decides to abrade a hole in some rock, it’s a sign that the geologists find the stuff interesting, or at least need to identify what’s at that spot to make sense of the immediately surrounding landscape.
I’m still working on a series of posts explaining all this in more detail - with neat pictures - but it’s going to take a while yet (we’ve made more than 30 of these holes, and they’ve shown us quite a few different things from start to finish!) Questions are welcome!
Thanks for the detailed write-up! It’s awesome how much we can learn (and have already learned) from the Mars rovers.