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Sols 4352-4354: Halloween Fright Night on Mars
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By NASA
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA’s Curiosity Mars rover sees its tracks receding into the distance at a site nicknamed “Ubajara” on April 30, 2023. This site is where Curiosity made the discovery of siderite, a mineral that may help explain the fate of the planet’s thicker ancient atmosphere.Credit: NASA/JPL-Caltech/MSSS New findings from NASA’s Curiosity Mars rover could provide an answer to the mystery of what happened to the planet’s ancient atmosphere and how Mars has evolved over time.
Researchers have long believed that Mars once had a thick, carbon dioxide-rich atmosphere and liquid water on the planet’s surface. That carbon dioxide and water should have reacted with Martian rocks to create carbonate minerals. Until now, though, rover missions and near-infrared spectroscopy analysis from Mars-orbiting satellites haven’t found the amounts of carbonate on the planet’s surface predicted by this theory.
Reported in an April paper in Science, data from three of Curiosity’s drill sites revealed the presence of siderite, an iron carbonate mineral, within the sulfate-rich rocky layers of Mount Sharp in Mars’ Gale Crater.
“The discovery of abundant siderite in Gale Crater represents both a surprising and important breakthrough in our understanding of the geologic and atmospheric evolution of Mars,” said Benjamin Tutolo, associate professor at the University of Calgary, Canada, and lead author of the paper.
To study the Red Planet’s chemical and mineral makeup, Curiosity drills three to four centimeters down into the subsurface, then drops the powdered rock samples into its CheMin instrument. The instrument, led by NASA’s Ames Research Center in California’s Silicon Valley, uses X-ray diffraction to analyze rocks and soil. CheMin’s data was processed and analyzed by scientists at the Astromaterials Research and Exploration Science (ARES) Division at NASA’s Johnson Space Center in Houston.
“Drilling through the layered Martian surface is like going through a history book,” said Thomas Bristow, research scientist at NASA Ames and coauthor of the paper. “Just a few centimeters down gives us a good idea of the minerals that formed at or close to the surface around 3.5 billion years ago.”
The discovery of this carbonate mineral in rocks beneath the surface suggests that carbonate may be masked by other minerals in near-infrared satellite analysis. If other sulfate-rich layers across Mars also contain carbonates, the amount of stored carbon dioxide would be a fraction of that needed in the ancient atmosphere to create conditions warm enough to support liquid water. The rest could be hidden in other deposits or have been lost to space over time.
In the future, missions or analyses of other sulfate-rich areas on Mars could confirm these findings and help us better understand the planet’s early history and how it transformed as its atmosphere was lost.
Curiosity, part of NASA’s Mars Exploration Program (MEP) portfolio, was built by NASA’s Jet Propulsion Laboratory, which is managed by Caltech in Pasadena, California. JPL leads the mission on behalf of NASA’s Science Mission Directorate in Washington.
For more information on Curiosity, visit:
https://science.nasa.gov/mission/msl-curiosity
News Media Contacts
Karen Fox / Molly Wasser
NASA Headquarters, Washington
202-358-1600
karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov
Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-2433
andrew.c.good@jpl.nasa.gov
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Last Updated Apr 17, 2025 Related Terms
Ames Research Center Astromaterials Curiosity (Rover) General Jet Propulsion Laboratory Mars Science Laboratory (MSL) Explore More
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Sols 4511-4512: Low energy after a big weekend?
This image was taken by Left Navigation Camera onboard NASA’s Mars rover Curiosity on Sol 4510 (2025-04-14 03:43:40 UTC). NASA/JPL-Caltech Written by Lauren Edgar, Planetary Geologist at USGS Astrogeology Science Center
Earth planning date: Monday, April 14, 2025
We all know the feeling: it’s Monday morning after a big weekend and you’re coming into the week wishing you’d had a little more time to rest and recharge. Well, Curiosity probably feels the same way today. Curiosity accomplished a lot over the weekend, including full contact science, a MAHLI stereo imaging test, testing the collection of ChemCam passive spectral data at the same time as data transmission with one of the orbiters, and some APXS and MAHLI calibration target activities, plus a long 57 m drive. It was great to see all of those activities in the plan and to see some great drive progress. But that means we’re a bit tight on power for today’s plan!
I was on shift as Long Term Planner today, and the team had to think carefully about science priorities to fit within our power limit for today’s plan, and how that will prepare us for the rest of the week. The team still managed to squeeze a lot of activities into today’s 2-sol plan. First, Curiosity will acquire Mastcam mosaics to investigate local stratigraphic relationships and diagenetic features. Then we’ll acquire some imaging to document the sandy troughs between bedrock blocks to monitor active surface processes. We’ll also take a Navcam mosaic to assess atmospheric dust. The science block includes a ChemCam LIBS observation on the bedrock target “Santa Margarita” and a long distance RMI mosaic of “Ghost Mountain” to look for possible boxwork structures. Then Curiosity will use the DRT, APXS and MAHLI to investigate the finely-laminated bedrock in our workspace at a target named “The Grotto.” We’ll also collect APXS and MAHLI data on a large nodule in the workspace named “Torrey Pines” (meanwhile the Torrey Pines here on Earth was shaking in today’s southern California earthquakes! All is well but it gave some of our team members an extra jolt of adrenaline right before the SOWG meeting). The second sol is focused on continuing our drive to the south and taking post-drive imaging to prepare for Wednesday’s plan.
Phew! Good job Curiosity, you made it through Monday.
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Sols 4509-4510: A weekend of long drives
This image was taken by Left Navigation Camera onboard NASA’s Mars rover Curiosity on Sol 4507 (2025-04-11 03:54:35 UTC). Written by Abigail Fraeman, Planetary Geologist at NASA’s Jet Propulsion Laboratory
Earth planning date: Friday, April 11, 2025
Curiosity is continuing to book it to the potential boxwork structures. The rover drove over 50 meters on Wednesday, and we plan to drive more than 50 meters again in today’s plan thanks to an unusually good viewshed that allows us to see far ahead. We’ve been able to see glimpses of the boxwork structures in the distance for a few weeks now, and I am really excited about being able to plan long drives that get us closer and closer. What will we find when we reach them?
Power was on everyone’s mind as we put the plan together today. The science team had lots of amazing ideas about observations to collect from our current location, but we had to carefully plan and prioritize them to make sure we didn’t use too much power and leave the rover battery lower than we’d like for Monday’s plan. Winter on Mars certainly keeps us on our toes! We ended up putting together what I think is a pretty good set of activities for the weekend. MAHLI, APXS, and ChemCam will all work together to observe a flat rock in front of us named “Iron Mountain.” MAHLI will also do an experiment with this rock, testing different combinations of camera positions to see which produces the best data to help us generate 3D models of the rock’s surface. I know rocks don’t have feelings, but if they did, I hope Iron Mountain can use this time to feel a bit like a movie star on the red carpet, getting photographed from all angles. Mastcam will also be photographing the surroundings, working with ChemCam’s RMI imager to take images the ridge containing boxwork structures named “Ghost Mountain,” and taking some solo shots of targets in the foreground named “Redondo Flat,” “Silverwood Sanctuary,” and the oft photographed Gould Mesa. Navcam, REMS, and DAN round out the science plan with some environmental observations. We’ll be getting one more science and engineering hybrid observation when we collect ChemCam passive spectral data of the instrument’s calibration target in parallel with one of our communication passes. This observation is part of a series of tests we’re doing to run rover activities in parallel with these passes, and if successful, will allow us to be more even more power efficient in the future.
We’re also celebrating a soliday this weekend, which means we only have a two-sol plan instead of our usual three as the Mars and Earth time zones re-align for the next few weeks. I’m looking forward to seeing where Curiosity drives next week.
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Sols 4507-4508: “Just Keep Driving”
NASA’s Mars rover Curiosity acquired this image using its Mars Hand Lens Imager (MAHLI), located on the turret at the end of the rover’s robotic arm, on April 9, 2025, Sol 4505 of the Mars Science Laboratory Mission, at 00:56:30 UTC. NASA/JPL-Caltech/MSSS Written by Natalie Moore, Mission Operations Specialist at Malin Space Science Systems
Earth planning date: Wednesday, April 9, 2025
Our drive from Monday’s plan was mostly successful, putting us ~22 meters down the “road” out of an expected 30 meters. A steering command halted the drive a little short when we tried to turn-in-place but instead turned into a rock, which also had the effect of making our position too unstable for arm activities. Oh well! APXS data has been showing the recent terrain as being pretty similar in composition, so the team isn’t complaining about trying again after another drive. Plus, keeping the arm stowed should give us a little more power to play with in the coming sols (an ongoing struggle this Martian winter).
Recently, my job on Mastcam has been to make sure our science imaging is as concurrent as possible with required rover activities. This strategy helps save rover awake time, AKA power consumption. Today we did a pretty good job with this, only increasing the total awake time by ~2 minutes even though we planned 52 images! Our imaging today included a mosaic of the “Devil’s Gate” ridge including some nodular bedrock and distant “Torote Bowl,” a mosaic of a close-by vein network named “Moonstone Beach,” and several sandy troughs surrounding the bedrock blocks we see here.
ChemCam is planning a LIBS raster on a vertical vein in our workspace named “Jackrabbit Flat,” and a distant RMI mosaic of “Condor Peak” (a butte to the north we’re losing view of). Our drive will happen in the 1400 hour on the first sol, hopefully landing us successfully 53 meters further into this new valley on our way to the boxwork structures to the west! Post-drive, we’re including a test of a “Post Traverse Autonav Terrain Observation” AKA PoTATO – an easy drop-in activity for ground analysis of a rover-built navigation map of our new terrain. Plus we get to say PoTATO a lot.
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