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NASA's SkyFall Mars helicopters will wear tiny capes

7 August 2026 at 17:07

Picture it: A swarm of tiny robot helicopters descends through a reddish-brown sky, landing gracefully on the Martian surface. What are they wearing? Tiny capes.

NASA's SkyFall mission will send a trio of mini rotorcraft to Mars equipped with ground penetrating radar technology which happens to look like little capes. These uniquely designed swaths of fabric look decidedly strange or even accidental in new videos from NASA's Jet Propulsion Laboratory (JPL) that show the little drones practice landing. But these capes are actually flexible antennae that will allow the craft to peer beneath the Red Planet's surface in search of water ice.

"The only way to detect shallow subsurface ice remotely is to fly close to the ground," Adrian Tang, SkyFall’s ground-penetrating radar lead instrument scientist at JPL, said in a statement on Thursday (Aug. 6). "By flying low and slow, a SkyFall helicopter could capture radar images that resolve the fine layering where dry soil gives way to ice, detecting its presence and mapping its extent."

Orbiting spacecraft have studied Mars for decades, imaging the planet and mapping it with radar. But from orbit, their radar is unable to see the first few feet of material just below the planet's surface — a zone where scientists expect to find shallow ice deposits mixed in with the rocks and dust. This work could be important for future astronauts who need to better understand the ground below their feet for safety reasons, and for future travelers searching for accessible ice to process for drinking water, oxygen and fuel.

Skyfall will follow in the footsteps of Ingenuity, the first rotorcraft on another world, which hitched a ride to Mars aboard NASA's Perseverance rover. The new choppers are based heavily on Ingenuity, which weighed just 4 pounds (1.8 kilograms) here on Earth. But Skyfall will be more capable than Ingenuity, whose main job was to show that choppers can explore the thin skies of Mars.

SkyFall's tiny cape ground-penetrating radar, which uses a type of flexible antenna called Vivaldi that was invented back in 1978, is designed to survey up to 16 feet (5 meters) below the Martian surface. The radar will be able to reach anywhere from several yards below the planet's surface to the uppermost layers of surface material.

And the antenna's unique design ensures that the SkyFall drones will be able to make these subsurface observations without damaging the equipment during landing.. The antenna is extremely lightweight, and the team miniaturized it to be both the right size and shape to fit the tiny helicopters, which sit just 6 inches (15 centimeters) above the ground at rest. The tricky thing was, the designers had to miniaturize the radar antennae while maintaining functionality. But they did just that, and these tiny radar capes will be able to bend and move out of the way as the rotorcraft do their thing, flying above and landing on the Red Planet.

"Although we managed to shrink the antenna quite a bit, it is about 1.5 times longer than the helicopter’s legs," Christine Gebara, SkyFall ground-penetrating radar mechanical lead at JPL, added in the statement.

"That means during landing, the Vivaldi has to bend out of the way — and if it lands on a rock, it bends even further," she added. "But when the helicopter takes off again, the antenna must spring back into place for data collection. Because SkyFall is expected to make dozens of flights exploring Mars, we needed an antenna that could repeatedly handle those pressures without losing its shape in flight."

A radar engineer works on a test antenna for the SkyFall mission’s ground-penetrating radar in the electromagnetic interference chamber at JPL.

A radar engineer at NASA JPL works to test the antenna on the SkyFall helicopter. (Image credit: NASA/JPL-Caltech)

To make these little capes capable of withstanding incredible feats on another world, the engineers behind the helicopters covered the antenna in layers of polyester and Vectran, a flexible (but incredibly strong) material that was previously used for the airbag that cushioned NASA's Spirit and Opportunity Mars rovers during their touchdowns in 2004. The antenna's shape is also reinforced with flexible fiberglass tape springs and a lightweight structure. In total, each antenna weighs a miniscule 5 ounces (142 grams).

But a crafty design isn't enough. Getting to Mars is no small feat, and NASA needs to be sure that these little helicopters and their gear are up to the challenge. So, in JPL's Environmental Test Laboratory, which recreates different elements of environments beyond Earth, the SkyFall team put the rotorcraft and its little radar antenna to the test. They bent and flexed the antenna over and over, recreating multiple landings on the surface, exposed the craft to extreme temperatures, and continually checked to make sure that, throughout this testing, the helicopter could still transmit and receive radar signals. At the end of this testing, the antenna had endured 200 simulated Mars landings and was still working just fine. That is more than twice the number of landings expected from the mission.

"This test checked every box it was supposed to and answered our biggest technical questions," Tang added. "While we still have work ahead of us before the antenna is fully flight-qualified, this was a major milestone, and the hardware performed exactly as expected."

The trio of SkyFall helicopters will put their radar capes to the ultimate test when they fly to Mars. NASA plans to launch this mission to the Red Planet in 2028 aboard NASA's Space Reactor-1 Freedom, the first nuclear fission-powered interplanetary spacecraft.

Une nouvelle ère commence : comment l'IA s'apprête à rendre la vie possible sur la Lune et Mars

6 August 2026 at 20:02
Et si l'IA ne se contentait plus d'assister l'exploration spatiale, mais en devenait l'architecture fondamentale ? Maintenance prédictive, autosuffisance sur Mars ou sur la Lune, défense orbitale, médecine autonome à des millions de kilomètres de tout secours : ce que prépare la prochaine...

Lessons for the future of NASA Mars exploration from a 1970s mission

6 August 2026 at 16:00

July 20 marked the 50th anniversary of one of the biggest robotic spaceflight achievements in NASA’s history: the landing of the Viking 1 spacecraft on Mars. It was the first […]

The post Lessons for the future of NASA Mars exploration from a 1970s mission appeared first on SpaceNews.

Curiosity rover spots mysterious honeycombs on Mars | Space photo of the day for Aug. 5, 2026

a reddish-brown landscape of soil and rocks covered in slightly raised hexagonal lines of nearly equal size

A close-up of the polygon fractures discovered by NASA's Curiosity Mars rover highlights their honeycomb-like textures. (Image credit: NASA/JPL-Caltech/MSSS)

NASA's Curiosity Mars rover spotted surprising shapes in the Red Planet soil while exploring a large valley.

What is it?

These images were captured on June 19 and 20, 2026, or the 4,930th and 4,931st Martian days of Curiosity's mission. They show honeycomb-like patterns referred to as "polygonal fractures" found in a valley on Mars known as Valle Grande. They measure about 1.5 to 3 inches (4 to 8 centimeters) across.

While Curiosity has seen other curious geometric patterns on Mars before, scientists were surprised by this most recent find.

"We've seen a lot of fascinating landscapes through Curiosity's eyes, but this sea of polygons took our breath away," project scientist Ashwin Vasavada of NASA's Jet Propulsion Laboratory said in a statement. "We measured their shapes and chemistry carefully and are hopeful there are clues in the data as to how these features formed."

a reddish-brown landscape of soil and rocks covered in slightly raised hexagonal lines of nearly equal size

A panorama taken by NASA's Curiosity Mars rover showing a large field of hexagonal shapes in the Martian soil. (Image credit: NASA/JPL-Caltech/MSSS)

Why is it incredible?

This field of polygons in Valle Grande extends as far as Curiosity's instruments could see, even around the base of a steep hill scientists named "Miraflores."

a reddish-brown landscape of soil and rocks covered in slightly raised hexagonal lines of nearly equal size

NASA's Curiosity Mars rover captured this sand-capped butte, nicknamed "Miraflores," estimated to be about 20 feet (6 meters) tall, on June 11, 2026. (Image credit: NASA/JPL-Caltech/MSSS)

While mission scientists have theories about how these structures form, it ultimately remains a mystery how they formed.

It's thought that changes in temperatures on Mars could have caused water to squeeze through sediment layers, but scientists will need to collect more data before they can reach a conclusive answer.

Mars dust is toxic. How will future astronauts deal with it?

5 August 2026 at 14:00

Planting boots on Mars is hard enough. But getting "breathing room" on the Red Planet without inhaling toxic dust is yet another issue.

Given NASA's plans to eventually put astronauts on the Red Planet, the agency assembled a Martian Dust Limit Working Group earlier this year to review what's known and unknown about the toxicological hazard to human crews from exposure to Mars dust. The ultimate goal was to establish a permissible exposure limit for humans on the Red Planet by compiling a comprehensive set of expert perspectives regarding Martian dust toxicology, exposure pathways and mitigation strategies.

The working group's conclusions reinforced the view that an initial Martian dust standard "must balance conservatism with operational feasibility while accommodating architectural and scientific uncertainty," the report states. Furthermore, the report explains, "as additional Martian data and toxicological research become available, this standard should be periodically revisited to ensure continued protection of crew health during human exploration of Mars."

Unique study

A panel member for that study was Brian Hynek professor in the Department of Earth Science and a research associate at the Laboratory for Atmospheric and Space Physics, both at the University of Colorado, Boulder.

"It was a unique study," Hynek told Space.com, conducted by NASA specialists, space medicine experts, habitat designers, including toxicologists, volcanologists and geologists. "The task was to help gauge health hazards to humans, both for short and long-term stays," he said.

Just highlighting the differences between the moon and Mars played a role, said Hynek. "The moon is worse in some ways and Mars is worse in other ways."

Disneyland of dust

To be sure, one outcome from Apollo moonwalkers – the "dusty dozen" – is that dealing with lunar dust proved to be troublesome, much more than expected. The aged moon is a Disneyland of dust and crews that went there attested to that fact.

Once out and about, moonwalkers coped with very fine, tiny particles composed of sharp, glassy material. Lunar dust stuck to everything it came in contact with; dust eroded their spacesuits, caused overheating on equipment and instrumentation, compromised seals on their spacesuits, even irritated the eyes and lungs of moonwalkers.

"On Mars, dust particles are a little more rounded, not as jagged and cutting into you. But then you have all the extra chemical components and minerals that you don't have on the moon, like really unhealthy perchlorates," Hynek said. "We can use the lunar knowledge, but Mars is a totally different place," he added.

helmets and white spacesuits covered in grey dust inside a cramped metallic cabin

At the conclusion of Apollo 17's mission in December 1972, moonwalking suits and space helmets are covered by lunar dust. (Image credit: NASA)

Heavy metals

Hynek noted that Martian dust is known to contain various carcinogens, such as silica and numerous heavy metals. He co-authored a recent paper on "Potential Health Impacts, Treatments, and Countermeasures of Martian Dust on Future Human Space Exploration."

"There's talk about growing crops on Mars," Hynek observed. "The martian soil is full of all these nasty chemicals. So the astronauts might get more exposure from what they are growing on Mars than the actual airborne dust," said Hynek.

Then there's the dust that will assuredly find its way into the habitat, Hynek said, so engineers are looking at filtering systems and just how much time will be required to clean the inside of the habitat.

"It's good to have the forethought and to start considering the Martian dust and its hazards. It poses a lot more health hazards than the lunar dust," Hynek concluded.

Learned our lesson

Joel Levine, a research professor in applied science at William and Mary in Williamsburg, Virginia, is a leading expert on lunar dust, engineering and safety concerns. He was not a panel member of the NASA report.

Levine cited earlier thinking from a recent National Academy of Sciences report on human exploration of Mars. Two goals noted in that 2026 report are Mars dust-related:

  • Determine what controls the onset and evolution of major dust storms, which dominate present-day atmospheric variability.
  • Characterize the effects of Martian dust on human physiology and hardware lifetime.

"This indicates that Mars dust is on the minds of mission planners! This is good news based on our experience with lunar dust on the Apollo landings," said Levine. "It looks like we learned our lesson about dust at future human landing sites."

Levine stated that Mars sample returns would be very helpful to characterize Martian dust samples for chemical composition and other qualities. "Unfortunately, it does not look like the Mars samples already collected will ever be returned to the Earth for analysis," he said.

reddish-orange soil and rocks

Martian dust seen on NASA's Perseverance rover on July 27, 2026 (Sol 1932) by the rover's Right Mastcam-Z camera. (Image credit: NASA/JPL-Caltech/ASU)

Major takeaways

Shaunna Morrison, an associate professor in the Department of Earth and Planetary Sciences at Rutgers University in New Jersey, served as a panel member on the Martian Dust Limit Working Group.

"One of the major takeaways from the Mars dust working group is that martian dust is a real crew-health and engineering issue, but it is also a tractable one if it is treated as a design requirement from the beginning," Morrison emphasized.

The worry is not that Mars dust is uniquely or catastrophically toxic based on what we know now, Morrison told Space.com.

"The concern is that future crews will be living and working in a closed habitat, repeatedly going outside, bringing dust back in on suits and equipment, in a low-humidity environment," said Morrison. That's a condition in which small particles are more prone to becoming airborne and potentially inhaled, she said, and potentially crew members being exposed to fine respirable particles over many days.

reddish-orange soil and rocks

A region-wide seasonal dust storm obscures the Jezero Crater in this image from NASA's Mars Perseverance rover, acquired using its Left Mastcam-Z camera on Aug. 20, 2024 (Sol 1244, or Martian day 1,244 of the rover's mission). (Image credit: NASA/JPL-Caltech/ASU)

Prevention first

Morrison said that a key point is that we do not have as yet returned samples of authentic airborne martian dust. So NASA has to build a conservative standard using the best available evidence: lunar dust toxicology, Mars simulant studies, and the very extensive chemical and mineralogical datasets from Mars rovers and landers, she pointed out.

"The best strategy is prevention first," Morrison said. "Keep as much dust as possible outside the habitat, remove it quickly when it gets in, monitor airborne particles, and design the system so crews are not relying on medical countermeasures after exposure," she advised.

NASA’s Curiosity Finds a Vast Sea of Mysterious Polygons on Mars

2 August 2026 at 12:23
NASA’s Curiosity Mars Rover Martian PolygonsCuriosity has found a vast sea of Martian polygons that may reveal how water and climate once reshaped the Red Planet. NASA’s Curiosity rover has encountered an enormous field of honeycomb-shaped fractures while climbing through a Martian valley known as “Valle Grande.” Each geometric feature measures roughly 1.5 to 3 inches (4 to 8 centimeters) [...]

NASA's Curiosity Mars Rover Discovers a Field of Honeycomb Textures

1 August 2026 at 22:39
NASA's Curiosity rover has sent back images of honeycomb-like textures called polygonal fractures, each one about 1.5 to 3 inches (4 to 8 centimeters) across. NASA reports: The mission has spotted small patches of these geometric shapes several times before, but nothing at the scale discovered in Valle Grande. In a 360-degree panorama that the rover captured on June 19 and 20, the 4,930th and 4,931st Martian days, or sols, of the mission, the polygonal shapes spread in all directions for as far as the rover can see... "[T]his sea of polygons took our breath away," said the mission's project scientist, Ashwin Vasavada of NASA's Jet Propulsion Laboratory in Southern California... Some of the polygons that the mission has spotted in the past clearly formed as mud cracks, though a variety of processes can contribute to their honeycomb textures, including cycles of warm and cold temperatures or compression that squeezed water out of the sediment when the surface was buried. These newly discovered polygons are among the many surprises Curiosity has trundled across since landing on Mars 14 years ago, on Aug. 5, 2012. Besides sulfur crystals, shiny meteorites, and other interesting geologic features, the rover has made major discoveries about the ancient Martian environment — most importantly, that it had the water, chemistry, and nutrients to support microbial life. Billions of years ago, lakes and streams dappled the lower foothills of Mount Sharp, a 3-mile-tall (5-kilometer-tall) mountain that Curiosity has been ascending since 2014. The rover has previously uncovered chemistry left over from Mars' watery history, including carbon-based molecules believed to be precursors to RNA and DNA, two nucleic acids that carry genetic information. Scientists have no way of knowing whether these organic molecules were created by biologic or geologic processes — either path is possible — but their discovery reconfirmed that ancient Mars had the right chemistry to support life. Dark, pebble-sized rocks also litter the area, NASA writes in a blog post, saying it's a "still-to-be-resolved question" as to whether they're bits of Mars that "floated" down from higher in the sediment layers, or "were ejected from distant impacts outside of Gale crater, or are meteorites from beyond Mars altogether."

Read more of this story at Slashdot.

« Cela nous a coupé le souffle » : une immense structure en nid-d’abeilles découverte sur Mars intrigue la Nasa

1 August 2026 at 12:27
Nous n'en sommes toujours qu'au début de l'exploration de la Planète rouge, aussi bien pour sa géologie que pour sa possible exobiologie. Cette exploration est grandement facilitée avec des machines, comme dans tout le Système solaire et comme l'avait prédit Arthur Clarke. Aujourd'hui, c'est...

EAGLE

31 July 2026 at 23:02

EAGLE

Explorer for Artemis Geology, Lunar, and Earth — a NASA satellite program to study surface biology and geology on Earth, with technologies that could support future missions to the Moon and Mars.

Future Mission

NASA’s EAGLE program — Explorer for Artemis Geology, Lunar, and Earth — will be a series of satellite missions studying surface properties using technologies for Earth observation that will also benefit future missions to the Moon and Mars, where they could identify critical resources and safe landing sites.

The satellites making up the first two EAGLE missions will study biology and geology on Earth’s surface to support agriculture, disaster response, and other needs. Each mission will carry a different instrument with capabilities that complement each other. The first mission (EAGLE-VSWIR) is scheduled to take flight in 2028.

Mission Type

Orbiter

Target

Earth, Moon, Mars

Launch

No earlier than 2028

Objective

Study surface composition and changes

  • EAGLE-VSWIR

    EAGLE-VSWIR (Visible to Shortwave Infrared) will observe the Earth’s surface every 16 days with a high-resolution imaging spectrometer, which measures light reflected from the planet’s surface, separating wavelengths across the visual and into the infrared spectrum. The patterns created by light being reflected or absorbed across this spectral range act like fingerprints, letting scientists identify the composition of the surface. 

    A similar instrument, NASA’s EMIT (Earth Surface Mineral Dust Source Investigation), has been monitoring Earth from the International Space Station since July 2022, characterizing the surface mineral composition of Earth’s arid lands, monitoring ecosystem status, and tracking health and safety hazards — such as methane leaks and acid mine drainage — among other applications.

    EAGLE-VSWIR will have 25 times more capability than EMIT has today. This technological leap will allow scientists to map surface deposits of critical and rare-earth minerals, strengthen food security, and aid wildfire prevention and recovery. It can also highlight environmental hazards such as oil spills or landslide risks, and monitor water quality and availability.

    Region of Nevada as observed by NASA's EMIT with spectrum on right edge
    The front of this image cube shows a region in Nevada observed by NASA’s EMIT imaging spectrometer; the cube’s sides show the spectral fingerprint for every point in the image and can be used to discover mineral resources. EAGLE-VSWIR will have 25 times greater performance beyond NASA’s current state-of-the-art EMIT.
    NASA/JPL-Caltech
  • EAGLE-TIR

    The EAGLE-TIR mission will provide Thermal InfraRed (TIR) imagery when it launches two to three years after EAGLE-VSWIR, measuring energy emitted from the surface and producing data that scientists can use to map temperature, composition, and critical mineral deposits. On Earth that would let researchers monitor wildfires and volcanic activity, track drought and water use by crops, study urban heat islands, observe the rates that snow or ice accumulates or melts, and better understand Earth’s resilient ecosystems.

    EAGLE-TIR follows on from ECOSTRESS (ECOsystem Spaceborne Thermal Radiometer Experiment on Space Station), which has been observing Earth from the International Space Station since 2018. ECOSTRESS was designed to study how different ecosystems respond to drought and water stress, and the data has provided a vital understanding of how plants’ water use changes throughout the day. Since ECOSTRESS also measures emitted energy in the thermal infrared, its surface-temperature products have also been used for urban planning and wildfire monitoring. 

    Further innovation and lessons learned from ECOSTRESS has led to EAGLE-TIR, which will carry a multi-band thermal radiometer. EAGLE-TIR’s great strength compared to existing missions is that it provides detailed imagery of the entire globe every two days, day and night, at multiple wavelengths not available from other instruments.

    Aerial view of Namib desert in Infrared captured by ECOSTRESS
    This image shows the minerals contained in Namibian dunes using ECOSTRESS data. EAGLE-TIR will have more spectral channels to enable even better mineral discrimination.
    NASA/JPL-Caltech
  • EAGLE Program

    By advancing vital techniques for measuring our planet’s surface composition, resources, and hazards, the EAGLE program addresses critical needs in Earth observation, with technologies that can also transfer to planetary exploration, where they’ll serve as pathfinders for future missions to the Moon and Mars.

    015B0489.NEF
    As the Artemis II crew came close to passing behind the Moon and experiencing a planned loss of signal, they captured this image of a crescent Earth setting on the Moon’s limb on April 6, 2026.
    NASA
Featured Video

EAGLE

NASA unveiled the EAGLE program as one part of its “Ignition” event on March 24, 2026, when it announced a wide-ranging series of transformative agencywide initiatives. With EAGLE (the Explorer for Artemis Geology, Lunar, and Earth missions), NASA will deploy breakthrough hyperspectral images across Earth with later missions anticipated for the Moon and Mars in rapid succession. On Earth they’ll identify critical minerals for national security, enable precision agriculture, and support disaster response. On Earth and at Mars they will locate critical minerals and resources such as ice for propellants, rare-earth elements for technology, and construction materials for habitats.

EMIT

EMIT (Earth Surface Mineral Dust Source Investigation) measures the mineral composition of Earth’s dust source regions, to help scientists understand how they heat or cool our planet.

Learn More About EMIT

ECOSTRESS

ECOSTRESS (ECOsystem Spaceborne Thermal Radiometer Experiment on Space Station) is accurately measuring the temperature of plants on Earth.

Learn More About ECOSTRESS

The post EAGLE appeared first on NASA Science.

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Join us for continuing coverage as our leaders discuss the agency's implementation of the National Space Policy and our plans to advance science and discover...

NASA Mars Rover Discovers Field of Mesmerizing Polygons

30 July 2026 at 17:15

A vast field of mesmerizing polygons has left Mars scientists enthralled.

Don’t be mistaken: NASA didn’t send a robot across the solar system so its eggheads could get a rundown in basic geometry. Instead, the Curiosity rover stumbled upon a stretch of the Martian valley called “Valle Grande” where the landscape is defined by honeycomb-shaped patterns ranging two to four inches in diameter.

These so-called “polygonal fractures” have been spotted elsewhere on the Red Planet, but never texturing an entire landscape at such a scale.

“We’ve seen a lot of fascinating landscapes through Curiosity’s eyes, but this sea of polygons took our breath away,” project scientist Ashwin Vasavada at NASA’s Jet Propulsion Laboratory said in a statement. “We measured their shapes and chemistry carefully and are hopeful there are clues in the data as to how these features formed.”

Curiosity has delivered a new 360-degree panorama from Mars. “We’ve seen a lot of fascinating landscapes through Curiosity’s eyes, but this sea of polygons took our breath away,” said the mission’s project scientist. 1/2 pic.twitter.com/G7sV6Xafkq

— NASA Mars (@NASAMars) July 29, 2026

The Curiosity rover stumbled on the polygon field while ascending the foothills of a three-mile-high mountain called Mount Sharp, where it’s been roaming since 2014. Captured with its Mastcam instrument, a panorama composed of 340 images taken back on June 19 show the hexagons dominating a huge stretch of the landscape. 

On Mars, polygonal textures are generally mud cracks. What created them hints at the planet’s fascinating geological history: the honeycombs can form as a result of water drying up and causing sediments to shrink, or they can be carved out by extreme temperature swings. By studying these features, scientists hope to piece together how flowing water once helped shape the Red Planet’s surface.

More on Mars: NASA Rover Finds “Complex Organic Matter” on Mars

The post NASA Mars Rover Discovers Field of Mesmerizing Polygons appeared first on Futurism.

MCMC Science

24 July 2026 at 22:46

MCMC Science

In addition to model development, the Mars Climate Modeling Center (MCMC) conducts cutting-edge scientific research on the past and present atmosphere and climate of Mars.

NASA Ames MCMC Logo Left Justified

The Mars Climate Modeling Center (MCMC) conducts atmospheric and climate science research using the NASA Ames Mars Global Climate Models (MGCMs), advancing our understanding of Mars’ climate today, in its ancient past, and as a target for future exploration.

Mars’ climate is governed by three interacting cycles — dust, water, and carbon dioxide (CO₂) — that vary across seasons and from year to year. MCMC scientists use the MGCMs to study these cycles and the processes that drive them, including:

  • Dust storms and dust transport – Investigating the mechanisms that lift, transport, and remove dust in the Martian atmosphere, including the onset and evolution of regional and global-scale dust storms.
  • Water and CO₂ cycles – Studying the seasonal exchange of water and CO₂ between the atmosphere, polar caps, and surface, and the clouds that form as a result.
  • Atmospheric dynamics – Examining circulation patterns, wave-mean flow interactions, and the extension of the MGCM into the middle atmosphere to better connect the lower and upper atmosphere.
  • Ancient Mars and habitability – Reconstructing past climate states, including the role of asteroid and comet impacts, to assess when and where conditions may have supported liquid water and habitability.
  • Mission support – Applying model results to landing site selection and characterization, atmospheric entry planning, and interpretation of data from current and past Mars missions.

This research is carried out by a team of civil servant and contractor scientists, postdoctoral researchers, and students, often in collaboration with universities and other NASA centers. You can read more about individual MCMC team members and their science on the Group Members page. A full list of MCMC research papers, conference presentations, and technical reports is available on the Publications page.

The post MCMC Science appeared first on NASA Science.

MCMC Webserver

24 July 2026 at 20:06

Model Webserver

The Mars Climate Modeling Center (MCMC) presents the webserver, a website for interactive plotting and downloading Mars Global Climate Model (MGCM) output.

Artist rendering of MCMC's MGCM cubed-sphere grid with an overlay of a surface temperature plot

The model visualization tool offers the most accessible introduction to Mars Global Climate Model (MGCM) data. It is an online dashboard that allows users to interactively plot, explore, and download model output stored on the NAS Data Portal (see the MGCM Output tab for more information).

GCM analysis tools

MGCM Webserver

You can explore, plot, and download the MGCM output through our user-friendly web interface.

Link to the Webserver
Screenshot showing the MCMC data portal web interface
The Data Portal Web Interface plotting surface temperature from MGCM output stored on the NAS Data Portal
NASA/Courtney Batterson

If you use the web interface in your research, please cite it as follows:

Web Interface (APA):

NASA Ames Mars Climate Modeling Center. (2024, August 14). Data Portal Web Interface [Web tool]. NASA Ames Research Center, NASA. https://data.nas.nasa.gov/mcmc/portals/web-interface/

Return to the MCMC homepage

Mars Climate Modeling Center (MCMC) Logo in the banner style
Mars Climate Modeling Center (MCMC) banner
NASA/Courtney Batterson

The post MCMC Webserver appeared first on NASA Science.

This Week In Space LIVE: The Viking Mars landings 50 years later

24 July 2026 at 13:00

Hey, Space Fans! Every weekend here at Space.com, you may have noticed we highlight the latest episode of the podcast This Week In Space, a TWiT show co-hosted by yours truly and my friend and colleague Rod Pyle, a space historian and editor of the National Space Society magazine Ad Astra.

This Week In Space episodes usually drop each Saturday, but this week we're doing something a bit different. To mark the 50th anniversary of NASA's Viking landings (Viking 1 touched down on Mars on July 20, 1976), Rod and I will host a special live taping of the podcast to discuss all things Martian starting at 1:30 p.m. EDT (1730 GMT). It should last up to 90 minutes.

Joining us on the podcast will be:

  • Dr. Pascal Lee, a planetary scientist, geologist and artist with the SETI Institute, Mars Institute and NASA Ames Research Center.
  • Dr. Penny Boston, an astrobiologist and speleologist (the study of caves) with the New Mexico Institute of Mining and Technology.

During our discussion, we'll touch on the personal and scientific impacts of NASA's Viking Mars landings and look at where Mars exploration may go in the modern age. We might even discuss the best places for the hunt for signs of life: the surface or inside Martian caves?

So if you're a Mars fan or a casual space aficionado, join us today at 1:30 p.m. EDT to get a detailed look at NASA's Viking Mars landings and their lasting impact on Martian exploration.

NASA’s MAVEN Illuminates New Understanding of Auroras at Mars

23 July 2026 at 16:19

This illustration depicts charged particles from a solar storm stripping away charged particles of Mars' atmosphere, one of the processes of Martian atmosphere loss studied by NASA's MAVEN mission, beginning in 2014.
This illustration depicts charged particles from a solar storm stripping away charged particles of Mars’ atmosphere, one of the processes of Martian atmosphere loss studied by NASA’s MAVEN mission.
NASA/GSFC

NASA MAVEN (Mars Atmosphere and Volatile Evolution) mission scientists have uncovered a key puzzle piece in understanding certain types of auroras on Mars, finding that they form in a similar way to Earth-based auroras.
 
Results published Thursday in Nature Communications show the same mechanism that circulates and catapults charged particles into Earth’s atmosphere is happening at Mars on much smaller scales because of differences in the two planets’ magnetic fields.
 
The MAVEN spacecraft, in orbit around Mars, experienced a loss of signal with ground stations on Earth on Dec. 6, 2025. On June 3, NASA declared the mission had concluded after finding the spacecraft to be unrecoverable. However, data from the mission is still being used to inform NASA science and future missions to Mars.
 
When the Sun’s magnetic field lines get close to Earth’s magnetosphere, the large magnetic bubble protecting the planet, they can reconnect and inject energy and mass throughout Earth’s magnetosphere and magnetotail, ultimately firing electrons back into the atmosphere to generate Earth’s auroras. This process, called the Dungey cycle, drives electrical currents, accelerates charged particles that create auroras, and controls the circulation of plasma in Earth’s magnetosphere and ionosphere.
 
This new study shows that a miniature version of the Dungey cycle is happening over Mars’ strong crustal magnetic fields, which gives scientists a better look into the physics of Martian auroras.
 
“We knew that magnetic reconnection was happening at Mars but did not expect it to be like the Dungey cycle,” said Shaosui Xu, lead author of the study and associate research physicist at the Space Sciences Laboratory at the University of California, Berkeley.
 
Mars does not have a global magnetic field like Earth. Earth’s magnetic field is created by our planet’s churning core, while Mars has numerous miniature magnetospheres that arise from intensely magnetized crust scattered around the planet.  These regions were formed around 4 billion years ago when lava cooled in the presence of Mars’ ancient global magnetic field, which has since disappeared due to intense solar wind stripping the planet’s atmosphere.
 
The MAVEN mission has observed highly localized auroras over these crustal fields, similar to Earth’s auroras at the poles, but it wasn’t until now that scientists could fully understand the physics of how they form. The study used several instruments aboard the MAVEN spacecraft to build up a picture of the Dungey-like behavior: the Magnetometer and Solar Wind Electron Analyzer instruments, which were used to determine the magnetic configuration and derive electrical currents, and the STATIC (Suprathermal and Thermal Ion Composition) instrument, which was used to measure plasma flows in the ionosphere.
 
“We really pushed the limit of STATIC to get the data we needed,” said Xu. “It was the final piece to the puzzle in understanding these localized auroras.”
 
The realization that a Dungey-like cycle was happening within these crustal magnetic fields answered the question of how the electrons were being energized to create the auroras. It also shows that a Dungey-like mechanism can happen on both large and small scales, giving more insight into where in the solar system this process could be taking place.
 
“This is a remarkable result that changes how we think of Martian auroras and is another important step toward understanding why Mars and Earth have evolved so differently despite being governed by the same underlying physics.” said Shannon Curry, MAVEN’s principal investigator and a research scientist at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder. “I am incredibly proud of our team’s work on this discovery and excited to uncover new insights into the Red Planet and its evolution.”
 
By finding out more about this process, scientists also are gaining a better understanding of how the solar environment interacts with the Red Planet as a whole, which is essential for future robotic and crewed missions.
 
“I remember in graduate school discussing with my advisor how the cycling of crustal magnetic fields could work at Mars,” said Xu. “It’s incredible to be part of the team that found the answer to that question.”
 
The MAVEN mission is part of NASA’s Mars Exploration Program portfolio. The mission’s principal investigator is based at the Laboratory for Atmospheric and Space Physics at the University of Colorado Boulder, which also is responsible for managing science operations and public outreach and communications. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the MAVEN mission. Lockheed Martin Space built the spacecraft and is responsible for mission operations. NASA’s Jet Propulsion Laboratory in Southern California provides navigation and Deep Space Network support.
 
For more information on NASA’s MAVEN mission, visit:
 
https://science.nasa.gov/mission/maven/
 
Karen Fox / Alana Johnson
Headquarters, Washington
240-285-5155 / 202-672-4780
karen.c.fox@nasa.gov / alana.r.johnson@nasa.gov
 
Lonnie Shekhtman
NASA’s Goddard Space Flight Center, Greenbelt, Md.
lonnie.shekhtman@nasa.gov

 

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