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Curiosity Blog, Sols 5016–5021: Fantastic Minerals and How To Detect Them NASA’s Mars rover Curiosity generated this close-up image of a brushed spot on bedrock (informally named “Salar de Vacas”), showing a jumble of roughly disc-shaped features as well as a divot generated by the brushing from the rover’s Dust Removal Tool (DRT). The features are about 3-4 millimeters across (about 0.12-0.16 inches) and about 1 millimeter thick (about 0.04 inches). Curiosity created the image using its Mars Hand Lens Imager (MAHLI), a close-up camera located on the turret at the end of the rover’s robotic arm, and an onboard focusing process that merges multiple images of the same target at different focus positions, creating a composite that brings as many features into focus as possible. Curiosity performed the focus merge on Sept. 16, 2026 — Sol 5016, or Martian day 5,016 of the Mars Science Laboratory Mission — at 02:14:02 UTC. NASA/JPL-Caltech/MSSSWritten by Lucy Lim, Planetary Scientist at NASA Goddard Space Flight Center
Earth planning Friday, Sept. 18, 2026
Curiosity surprised us at the beginning of the week with a change in rock texture — instead of the finely layered bedrock blocks we’ve been seeing in our recent sulfate unit workspaces, suddenly we were looking at blocks covered (and likely filled) with a jumble of small disc-shaped lumps. We’ve seen somewhat similar features before much earlier in the mission — for example, close to the Pahrump Hills back in the Murray mudstones, and they’re sometimes seen in Earth rocks as well, especially in settings in which minerals were precipitating from an evaporating fluid. The disc-like shapes could be created by the growth habits of a specific crystalline mineral that is known to grow into similar shapes, or they could be bits of a harder rock layer that broke up and collected here. We planned Mastcam and MAHLI imaging for more morphological detail on the jumbled disc blocks (“Yungay,” “Chiu Chiu”) as well as LIBS (“Puya Raimondii,” “Liolaemus Tacnae,” “Pisqu Warkatana”) and APXS (“Salar de Vacas”) to investigate their composition.
Ongoing long-distance imaging projects were furthered by ChemCam long-distance remote imager (RMI) and Mastcam mosaics of the buttes on either side of Valle Grande. These “cutaway”-view images of the strata above the rover will help us map sedimentary structures in these upcoming units and understand how these rocks formed and eroded. Views of more recent erosional deposits will also help us to understand the formation of Valle Grande itself.
In order to identify minerals, Curiosity needs data from the CheMin X-ray diffraction instrument, which means a drill campaign. We’ve driven over a kilometer since our last drill site at Campo Marte, and this will be our first drill above the erosional supersurface. The Wednesday plan’s drive brought us up next to a promising drill workspace a little beyond where we saw the disc-shaped features discussed above (imaged as “Torres del Paine” by Mastcam) and Friday’s planning included site characterization with the instruments on Curiosity’s arm (“Alberta Wild Rose,” “Moonraker Mountain”), ChemCam LIBS (“Osoyoos”), and Mastcam (“Trincomali Channel,” “Yellow Lady’s Slipper”). The team also selected a specific drill target and planned a very short drive to bring it in range of the arm — first for contact science and then, if all goes well, for the preload test and drill.
I’ll be back on planning on Monday as Geology and Mineralogy Science Theme Lead for Drill Sol 1 (Triage Contact Science) and we’ll see how things go from there!
Want to read more posts from the Curiosity team?
Visit Mission Updates
Want to learn more about Curiosity’s science instruments?
Visit the Science Instruments page
NASA’s Curiosity rover at the base of Mount Sharp NASA/JPL-Caltech/MSSSShare
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