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Curiosity Blog, Sols 4641-4648: Thinking Outside and Inside the ‘Boxwork’

Curiosity Blog, Sols 4641-4648: Thinking Outside and Inside the ‘Boxwork’

  • Curiosity Rover Explores Boxwork Unit: The Mars rover Curiosity has been exploring the boxwork unit, investigating both the ridges and hollows to better characterize them and understand how they may have formed.
  • Remote Science and Contact Science: The rover planners conducted remote science, contact science, and driving in each plan, including imaging, ChemCam LIBS, and MAHLI/APXS observations on various targets.
  • Challenging Drives: Curiosity faced challenging drives, particularly on Wednesday’s plan, where it had to overcome tilts above 20 degrees and navigate through dusty terrain with limited visibility.
  • New Discoveries: The rover planners found one spot after a lot of looking that was suitable for brushing, and they conducted DRT, APXS, and MAHLI observations on this target named “San Jose” and another rock named “Malla Qullu”.
  • Next Steps: After a week of exploring the boxwork unit, Curiosity will continue its mission to understand the geology and potential habitability of Mars, with upcoming plans including imaging and contact science targets.

4 min read

Curiosity Blog, Sols 4641-4648: Thinking Outside and Inside the ‘Boxwork’

A grayscale photo from the Martian surface shows a very rough, rocky ridge cutting horizontally across the image, about a third of the way down the frame from the top. Medium gray, like all the surrounding terrain, the ridge is covered in flat rocks with jagged fractures separating them, and it fills the bottom two-thirds of the frame. Above that in the image, beyond the ridge, the ground is mostly covered in what looks like fine sand, with scattered small rocks poking up. The sand is in numerous small dunes and ripples, looking like it had been sculpted by wind or water.
NASA’s Mars rover Curiosity acquired this image using its Left Navigation Camera on Aug. 28, 2025 — Sol 4643, or Martian day 4,643 of the Mars Science Laboratory mission — at 20:45:52 UTC.
NASA/JPL-Caltech

Written by Ashley Stroupe, Mission Operations Engineer and Rover Planner at NASA’s Jet Propulsion Laboratory

Earth planning week: Aug. 25, 2025.

This week Curiosity has been exploring the boxwork unit, investigating both the ridges and the hollows to better characterize them and understand how they may have formed. We’ve been doing lots of remote science, contact science, and driving in each plan. In addition, we have our standard daily environmental observations to look at dust in the atmosphere. We can still see distant targets like the crater rim, but temperatures will soon begin to warm up as we start moving into a dustier part of the year. And after each drive, we also use AEGIS to do some autonomous target selection for ChemCam observations. I was the arm rover planner for the 4645-4648 plan on Friday.

For Monday’s plan (sols 4641-4642), after a successful weekend drive Curiosity began on the edge of a boxwork ridge. We did a lot of imaging, including Mastcam mosaics of “El Alto,” an upturned rock near a wheel, the ridge forming the south side of the Mojo hollow, “Sauces,” our contact science target, and “Navidad,” an extension of our current workspace. We also took ChemCam LIBS of Sauces and an RMI mosaic. The rover planners did not find any bedrock large enough to brush, but did MAHLI and APXS on Sauces. Ready to drive, Curiosity drove about 15 meters (about 49 feet) around the ridge to the south and into the next hollow, named “Mojo.” 

In Wednesday’s plan (sols 4643-4644), Curiosity was successfully parked in the Mojo hollow. We started with a lot of imaging, including Mastcam mosaics of the ridges around the Mojo hollow, a nearby trough and the hollow floor to look for regolith movement. We also imaged a fractured float rock named “La Laguna Verde.” ChemCam planned a LIBS target on “Corani,” a thin resistant clast sticking out of the regolith, a RMI mosaic of a target on the north ridge named “Cocotoni,” and a long-distance RMI mosaic of “Babati Mons,” a mound about 100 kilometers (about 62 miles) away that we can see peeking over the rim of Gale crater! With no bedrock in the workspace, the rover planners did MAHLI and APXS observations on a regolith target named “Tarapacá.” The 12-meter drive in this plan (about 39 feet) was challenging; driving out of the hollow and up onto the ridge required the rover to overcome tilts above 20 degrees, where the rover can experience a lot of slip. Also, with the drive late in the day, it was challenging to determine where Curiosity should be looking to track her slip using Visual Odometry without getting blinded by the sun or losing features in shadows. Making sure VO works well is particularly important on drives like this when we expect a lot of slip. 

Friday’s plan, like most weekend plans, was more complex — particularly because this four-sol plan also covers the Labor Day holiday on Monday. Fortunately, the Wednesday drive was successful, and we reached the desired parking location on the ridge south of Mojo for imaging and contact science. The included image looks back over the rover’s shoulder, where we can see the ridge and hollow. We took a lot of imaging looking at hollows and the associated ridges. We are taking a Mastcam mosaic of “Jorginho Cove,” a target covering the ridge we are parked on and the next hollow to the south, “Pica,” a float rock that is grayish in color, and a ridge/hollow pair named “Laguna Colorada.” We also take ChemCam LIBS observations of Pica and two light-toned pieces of bedrock named “Tin Tin” and ”Olca.” ChemCam takes RMI observations of “Briones,” which is a channel on the crater rim, “La Serena,” some linear features in the crater wall, and a channel that feeds into the Peace Vallis fan. 

After a week of fairly simple arm targets, the rover planners had a real challenge with this workspace. The rocks were mostly too small and too rough to brush, but we did find one spot after a lot of looking. We did DRT, APXS, and MAHLI on this spot, named “San Jose,” and also did MAHLI and APXS on another rock named “Malla Qullu.” This last drive of the week is about 15 meters (about 49 feet) following along a ridge and then driving onto a nearby one.

A rover sits on the hilly, orange Martian surface beneath a flat grey sky, surrounded by chunks of rock.
NASA’s Mars rover Curiosity at the base of Mount Sharp
NASA/JPL-Caltech/MSSS

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Last Updated

Sep 04, 2025

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Q. What is Curiosity’s current mission objective?
A. Curiosity has been exploring the boxwork unit, investigating both the ridges and the hollows to better characterize them and understand how they may have formed.

Q. What was the rover’s plan for Monday (Sols 4641-4642)?
A. The rover began on the edge of a boxwork ridge, doing a lot of imaging, including Mastcam mosaics of several targets, ChemCam LIBS of Sauces, and MAHLI and APXS on Sauces.

Q. What was the challenge faced by the rover planners in Wednesday’s plan (Sols 4643-4644)?
A. The rover planners had a real challenge with this workspace because the rocks were mostly too small and too rough to brush, but they did find one spot after a lot of looking.

Q. What was the rover’s drive distance in Friday’s plan?
A. The rover drove about 15 meters (about 49 feet) following along a ridge and then driving onto a nearby one.

Q. What is the purpose of AEGIS on Curiosity?
A. AEGIS is used to do some autonomous target selection for ChemCam observations after each drive.

Q. What was the rover’s parking location in Wednesday’s plan (Sols 4643-4644)?
A. The rover successfully parked in the Mojo hollow, starting with a lot of imaging and then doing MAHLI and APXS on a regolith target named “Tarapacá”.

Q. How did Curiosity overcome tilts above 20 degrees during its drive?
A. The rover had to overcome tilts above 20 degrees by driving out of the hollow and up onto the ridge, which required careful planning and execution.

Q. What is the purpose of ChemCam LIBS on Curiosity?
A. ChemCam LIBS (Laser Induced Breakdown Spectroscopy) is used to analyze the chemical composition of rocks and targets.

Q. How did the rover planners select targets for ChemCam observations in Friday’s plan?
A. The rover planners selected targets using AEGIS, which helped them choose suitable locations for ChemCam observations.

Q. What was the significance of the 12-meter drive in Wednesday’s plan (Sols 4643-4644)?
A. The 12-meter drive was challenging because it required the rover to overcome tilts above 20 degrees and navigate through a dusty environment, which made it difficult to determine where the rover should be looking using Visual Odometry.