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Description

NASA’s Curiosity Mars rover discovered these bumpy, pea-sized nodules while exploring a region filled with boxwork formations — low ridges standing roughly 3 to 6 feet (1 to 2 meters) tall with sandy hollows in-between. This mosaic is made up of 50 individual images taken by Curiosity’s Mars Hand Lens Imager (MAHLI), a camera on the end of the rover’s robotic arm, on Aug. 21, 2025, the 4,636th Martian day, or sol, of the mission. Ten images at different focus settings were taken at each of five locations to produce a sharp mosaic. The images were stitched together after being sent back to Earth.

Figure A is the same image with a small scale bar added to the right-hand side.

Nodules like these have been seen many times before on the Red Planet, including by Curiosity. They were made by minerals left behind as water dried billions of years ago. Crisscrossing the surface for miles, the boxwork formations suggest ancient groundwater flowed on this part of the Red Planet later than expected, raising new questions about how long microbial life could have survived on Mars billions of years ago, before rivers and lakes dried up.

The boxwork ridgetops often include a dark line the team refers to as “central fractures,” where groundwater originally seeped through a rock crack, allowing minerals to concentrate. Surprisingly, the mission did not find nodules near these central fractures. Instead, they were found along the walls of the ridges and in the hollows between them. The wavy ridges between the groups of nodules are mineral veins made of calcium sulfate, also deposited by groundwater.

Curiosity 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 as part of NASA’s Mars Exploration Program portfolio. MAHLI was built by Malin Space Science Systems in San Diego.

To learn more about Curiosity, visit:

science.nasa.gov/mission/msl-curiosity

Description

NASA’s Curiosity Mars rover captured this panorama of boxwork formations — the low ridges seen here with hollows in between them — using its Mastcam on Sept. 26, 2025, the 4,671st Martian day, or sol, of the mission. These boxwork formations were created billions of years ago when water leaked through rock cracks. Minerals carried into the cracks later hardened; after eons of windblown sand eroding away the softer rock, the hardened ridges were left exposed.

The panorama is made up of 179 individual images that were stitched together after being sent back to Earth. This natural color view is approximately how the scene would appear to an average person if they were on Mars. 

Curiosity 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 as part of NASA’s Mars Exploration Program portfolio. Malin Space Science Systems in San Diego built and operates Mastcam.

For more about Curiosity, visit:

science.nasa.gov/mission/msl-curiosity

For about six months, NASA’s Curiosity Mars rover has been exploring a region full of geologic formations called boxwork, low ridges standing roughly 3 to 6 feet (1 to 2 meters) tall with sandy hollows in between. Crisscrossing the surface for miles, the formations suggest ancient groundwater flowed on this part of the Red Planet later than scientists expected. This possibility raises new questions about how long microbial life could have survived on Mars billions of years ago, before rivers and lakes dried up and left a freezing desert world behind.

The boxwork formations look like giant spiderwebs when viewed from space. To explain the shapes, scientists have proposed that groundwater once flowed through large fractures in the bedrock, leaving behind minerals. Those minerals then strengthened the areas that became ridges while other portions without mineral reinforcement were eventually hollowed out by wind.

Until Curiosity arrived at this region, however, no one could be sure what these formations looked like up close, and there were even more questions about how they were made.

Unpacking boxwork

Although Earth also has boxwork ridges, they’re rarely taller than a few centimeters and are usually found in caves or in dry, sandy environments. The Curiosity team wanted to get a close look at the Martian formations and gather more data. This posed a real challenge for rover drivers: They needed to send instructions to Curiosity, an SUV-size vehicle that weighs nearly a ton (899 kilograms), so that it could roll across the tops of ridges not much wider than the rover itself.

“It almost feels like a highway we can drive on. But then we have to go down into the hollows, where you need to be mindful of Curiosity’s wheels slipping or having trouble turning in the sand,” said operations systems engineer Ashley Stroupe of NASA’s Jet Propulsion Laboratory in Southern California, which built Curiosity and leads the mission. “There’s always a solution. It just takes trying different paths.”

For scientists, the challenge is piecing together how such a vast network of boxwork could exist on Mount Sharp, the 3-mile-tall (5-kilometer-tall) mountain the rover has been ascending. Each layer of the mountain formed in a different era of Mars’ ancient, changing climate. The higher Curiosity goes, the more the landscape bears signs that water was drying out over time, with occasional wet periods that saw the return of rivers and lakes.

“Seeing boxwork this far up the mountain suggests the groundwater table had to be pretty high,” said Tina Seeger of Rice University in Houston, one of the mission scientists leading the boxwork investigation. “And that means the water needed for sustaining life could have lasted much longer than we thought looking from orbit.”

Previous orbital imagery included one crucial piece of evidence: dark lines running across the “spiderwebs.” In 2014, it was proposed that these lines might be what are known as central fractures, where groundwater seeped through rock cracks and allowed minerals to concentrate. Investigating the ridges up close, Curiosity found that these lines are in fact fractures, lending weight to that hypothesis.

The rover also discovered bumpy textures called nodules, an obvious sign of past groundwater that has been spotted many times by Curiosity and other Mars missions. Unexpectedly, these nodules were not found near the central fractures, but along a ridge’s walls and the hollows between them.

“We can’t quite explain yet why the nodules appear where they do,” Seeger said. “Maybe the ridges were cemented by minerals first, and later episodes of groundwater left nodules around them.”

Roving laboratory

A major part of Curiosity’s science centers on rock samples collected by the rock-pulverizing drill on the end of the rover’s robotic arm. The resulting powder can be trickled into complex science instruments in the vehicle’s body for analysis.

Last year, three samples from the boxwork region — one from a ridgetop, one from bedrock within a hollow, and one from a transitional area before Curiosity reached the ridges — were collected by the drill and analyzed with X-rays and a high-temperature oven. The X-ray analyses found clay minerals in the ridge and carbonate minerals in the hollow, providing additional clues to help understand how these features formed.

The mission recently collected a fourth sample, which was analyzed with a special technique reserved for the most intriguing science targets: After the pulverized rock went into the rover’s high-temperature oven, chemical reagents reacted with the sample to conduct what is called wet chemistry. The resulting reactions make it easier to detect certain organic compounds, carbon-based molecules important to the formation of life.

Sometime in March, Curiosity will leave the boxwork formations behind. The whole region is part of a layer on Mount Sharp enriched in salty minerals called sulfates, which formed as water was drying out on Mars. Curiosity’s team plans to continue exploring this sulfate layer for many miles in the coming year, learning more about how the ancient Red Planet’s climate changed billions of years ago.

More about Curiosity

Curiosity 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 as part of NASA’s Mars Exploration Program portfolio.

To learn more about Curiosity, visit:

science.nasa.gov/mission/msl-curiosity

News Media Contacts

Andrew Good
Jet Propulsion Laboratory, Pasadena, Calif.
818-393-2433
andrew.c.good@jpl.nasa.gov

Karen Fox / Molly Wasser
NASA Headquarters, Washington
240-285-5155 / 240-419-1732
karen.c.fox@nasa.gov / molly.l.wasser@nasa.gov

2026-013

NASA’s Perseverance Rover approaches Mars in this Feb. 18, 2020, top-down still image captured by a camera on the rover’s descent stage.

Perseverance is searching for signs of ancient microbial life, to advance NASA’s quest to explore the past habitability of Mars. NASA chose Jezero Crater as the landing because scientists believe the area was once flooded with water and was home to an ancient river delta. In summer 2024, the rover collected a sample from the “Chevaya Falls” rock which was found to have potential biosignatures — clues that suggest past life may have been present, but that require more data or further study before any conclusions about the absence or presence of life.

In addition to making discoveries on Mars, the rover itself is demonstrating technological advances: A new technology developed at NASA’s Jet Propulsion Laboratory in Southern California enables Perseverance to figure out its whereabouts without calling humans for help. Dubbed Mars Global Localization, the technology features an algorithm that rapidly compares panoramic images from the rover’s navigation cameras with onboard orbital terrain maps.

Image credit: NASA/JPL-Caltech

Forty million years ago, a star in a nearby galaxy exploded, spewing material across space and generating a brilliant beacon of light. That light traveled across the cosmos, reaching Earth June 29, 2025, where it was detected by the All-Sky Automated Survey for Supernovae. Astronomers immediately turned their resources to this new supernova, designated 2025pht, to learn more about it. But one team of scientists instead turned to archives, seeking to use pre-supernova images to identify exactly which star among many had exploded. And they succeeded.

Images of galaxy NGC 1637 taken by NASA’s James Webb Space Telescope showed a single red supergiant star located exactly where the supernova now shines. This represents the first published detection of a supernova progenitor by Webb. The results were published in the Astrophysical Journal Letters.

“We’ve been waiting for this to happen – for a supernova to explode in a galaxy that Webb had already observed. We combined Hubble and Webb data sets to completely characterize this star for the first time,” said lead author Charlie Kilpatrick of Northwestern University.

Image: SN 2025pht in NGC 1637

Case of missing red supergiants

By carefully aligning Hubble and Webb images taken of NGC 1637, the team was able to identify the progenitor star in images taken by Webb’s MIRI (Mid-Infrared Instrument) and NIRCam (Near-Infrared Camera) in 2024. They found that the star appeared surprisingly red – an indication that it was surrounded by dust that blocked shorter, bluer wavelengths of light.

“It’s the reddest, most dusty red supergiant that we’ve seen explode as a supernova,” said graduate student and co-author Aswin Suresh of Northwestern University. 

This excess of dust could help explain a long-standing problem in astronomy that could be described as the case of the missing red supergiants. Astronomers expect the most massive stars that explode as supernovas to also be the brightest and most luminous. So, they should be easy to identify in pre-supernova images. However, that hasn’t been the case. 

One potential explanation is that the most massive aging stars are also the dustiest. If they’re surrounded by large quantities of dust, their light could be dimmed to the point of undetectability. The Webb observations of supernova 2025pht support that hypothesis.

“I’ve been arguing in favor of that interpretation, but even I didn’t expect to see it as extreme as it was for supernova 2025pht. It would explain why these more massive supergiants are missing because they tend to be more dusty,” said Kilpatrick.

Carbon “burps”

The team was not only surprised by the amount of dust, but also by its composition. Applying computer models to the Webb observations indicated that the dust is likely carbon-rich, when astronomers would have expected it to be more silicate-rich. The team speculates that this carbon might have been dredged up from the star’s interior shortly before it exploded.

“Having observations in the mid-infrared was key to constraining what kind of dust we were seeing,” said Suresh.

The team now is working to look for similar red supergiants that may explode as supernovas in the future. Observations by NASA’s upcoming Nancy Grace Roman Space Telescope may help this search. Roman will have the resolution, sensitivity, and infrared wavelength coverage to not only see these stars, but also potentially witness their variability as they “burp” out large quantities of dust near the end of their lives.

The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).

To learn more about Webb, visit:

https://science.nasa.gov/webb

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