NASA is playing an important role in JAXA’s (Japan Aerospace Exploration Agency) MMX (Martian Moons eXploration) mission, to advance our understanding of Mars’ moons and build on the agency’s long history of exploring the Red Planet.

The mission aims to characterize and determine the origin of Mars’ moons Phobos and Deimos and deliver a sample of Phobos to Earth. The MMX spacecraft is targeting launch from JAXA’s Tanegashima Space Center in Japan at 3:41 p.m. EDT on Monday, Oct. 19 (4:41 a.m. JST on Tuesday, Oct. 20).

“The samples from MMX will bring forth paradigm-shifting science on the Mars system for generations to come, especially as NASA prepares to send the first humans to Mars,” said Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters in Washington. “The NASA-JAXA sample curation partnership is extremely valuable, and I am proud that NASA Science is supporting MMX sample curation and will be sharing portions of these samples for study as we continue to expand humanity’s understanding of the universe for the benefit of all.”

NASA’s contributions to the mission include the Mars-moon Exploration with Gamma rays and Neutrons (MEGANE) spectrograph instrument, the Pneumatic Sampler (P-Sampler) technology demonstration, and communications and navigation support from the agency’s Deep Space Network, as well as funding United States scientists participating on the MMX science team.

Scientists have long debated the origin of Mars’ two moons. The data and samples collected by the MMX mission will help answer essential questions about the origins of these moons and the history of the solar system.

“Phobos and Deimos may be the remains of a massive impact on Mars that sent material into orbit around the planet, or they could be ancient asteroids that were captured by Mars’ gravity billions of years ago,” said Tom Statler, MMX program executive and program scientist at NASA Headquarters. “Having the answer will help illuminate that early era when Earth and the other inner planets may have been acquiring much of their water and organic compounds.”

The MEGANE (pronounced meh-GAH-nay, the Japanese word for eyeglasses) spectrograph will help scientists “see” what Phobos is made of by measuring neutrons and gamma rays emitted from the moon’s surface and determining its chemical elemental composition, which will provide important clues about its origin.

Mounted on one of the spacecraft’s landing legs, the P-Sampler is designed to collect a ground sample from Phobos. The system gathers surface material using bursts of high-pressure nitrogen gas, complementing JAXA’s C-Sampler, which will extract cores from a few inches deeper. NASA will obtain and curate about 15% of the total returned sample at the agency’s Johnson Space Center Astromaterials Lab in Houston, making it available for research for decades.

Another key part of NASA’s contribution to MMX is its scientific partnership with JAXA. NASA-supported researchers are working alongside international colleagues to help reveal the story of Phobos and will use mission data and returned samples to uncover new clues about the moon’s origin and the evolution of the Mars system.

The MMX spacecraft will arrive at Mars in August 2027 to begin its survey of the Red Planet’s two moons. After surveying Phobos in detail, the spacecraft will collect a sample of the moon’s surface no earlier than December 2028 and deliver it to Earth in 2031.

The MEGANE instrument was developed by the Johns Hopkins Applied Physics Laboratory. Honeybee Robotics, a Blue Origin company, developed the spacecraft’s pneumatic sampler mechanism. NASA’s contributions to the MMX mission were developed under the agency’s Discovery Program. The Discovery Program is managed by NASA’s Marshall Space Flight Center in Huntsville, Alabama, for the agency’s Science Mission Directorate in Washington.

For more information about the MMX mission, visit:

https://science.nasa.gov/mission/mmx

Karen Fox / Alana Johnson
Headquarters, Washington
240-285-5155 / 202-672-4780
[email protected] / [email protected]

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This NASA Hubble Space Telescope image features the edge-on, intermediate spiral galaxy NGC 1827, located roughly 37 million light-years away in the constellation Columba, the Dove. Hubble captured the image as part of a survey looking at 260 satellite galaxies around 22 Milky Way-like host galaxies within a radius of about 32 million light-years from Earth. Hubble has already observed 111 of these satellite galaxies. The remaining galaxies will take an additional 149 Hubble orbits, one orbit for each galaxy, to observe.

The image, taken with Hubble’s Advanced Camera for Surveys, reveals bright-blue regions along the galaxy’s disk dotted with dark dust lanes where new stars are likely forming. A bright foreground star appears just to the left of the galaxy’s bright central bulge but is located between us and the galaxy. Its four diffraction spikes are the result of light bending around the internal supports that hold Hubble’s secondary mirror.

Low-mass galaxies like the ones in this Hubble observing program provide a way to test the predictions of cosmological models on small scales, which struggle to match observations. The data Hubble gathers will help us better understand and characterize the properties of low-mass galaxies in Milky Way-like systems, allowing researchers to refine cosmological models.

Media Contact:

Claire Andreoli
NASA’s Goddard Space Flight Center, Greenbelt, MD
[email protected]

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3 Min Read

I Am Artemis: Allison Mjoen

As the supercooled propellant flowed into the core stage, and NASA’s SLS (Space Launch System) rocket roared to life, Allison Mjoen and her family watched with awe and pride. Mjoen, NASA’s operations manager for the agency’s Exploration Ground Systems Program, helped shape the systems and ground operations that will one day send humans back to the Moon. Over her 20-year career at NASA’s Kennedy Space Center in Florida, she supported missions across the Space Shuttle Program, the International Space Station, and now she is applying that experience to Artemis.

April 1, 2026, was a bright, crystal-clear day along the Florida Space Coast. The sunlight seemed to sharpen every color along the horizon. As Mjoen and her children counted down and the crowd’s voices rose around them, the rumble of the SLS rocket intensified beneath their feet. For her children, it was the chance to see what their mom had helped make possible. For Mjoen, it was a moment she would never forget.

That moment also offered a pause for reflection on the work that led her there. As the spacecraft offline operations manager, Mjoen coordinates the work that happens long before launch day. By supporting the ground systems’ senior vehicle operations manager, Matt Czech, she develops integration plans and oversees ground operations for Artemis vehicle processing, focusing on booster and Orion spacecraft operations.

Mjoen began her career as a flight crew systems engineer with United Space Alliance supporting the Space Shuttle Program. Her team handled mission-specific cabin configurations, including the food, spacesuits, cargo, and payloads astronauts needed aboard the shuttle.

After the Space Shuttle Program retired, she supported the International Space Station Program as a payload integration engineer. In this role, she connected experiment investigators with the organizations developing their hardware. She later worked in the Project Office on the Test and Operations Support Contract before joining NASA’s Operations Project Engineering Office, where she served as the Spacecraft Payloads Integration and Evolution Element lead for Artemis I.

“Early on, I thought every decision had to be perfect, but everything is an opportunity to learn, especially the tasks that seem unrelated at the time. It’s about staying curious, working hard, building relationships, and trusting that each step is preparing you for the next one.

Allison Mjoen

Operations Manager, NASA's Exploration Ground Systems

That preparation took on new meaning when she first supported integrated firing room operations as a certified operations project engineer during Artemis I. Earning the certification was a milestone. Applying it during real time operations brought a new level of responsibility.

“Every decision and communication directly supported the integrated team’s ability to execute safely and properly implement the test procedure,” said Mjoen.

Working at the integration console underscored the importance of preparation, collaboration and trust — lessons she carries into her work coordinating across teams today.

“I get to collaborate everyday with incredibly talented and dedicated people who are all working toward the same goal. It’s especially rewarding to know that our collective efforts directly contribute to the success of the mission.”

Allison Mjoen

Operations Manager, NASA's Exploration Ground Systems

For Mjoen, the shared experience is part of what makes Artemis so important. As the Artemis program continues, she looks forward to another moment families will be able to share as astronauts return to the lunar surface.

“That single moment captured the imagination of people around the world and showed what is possible when we come together for a bold goal,” she said of the first Apollo Moon landing. “Artemis is creating that kind of moment for a whole new generation, and this time to stay.”

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August 2026 Composite

October 11, 2026

August 2026 CompositeOctober 11, 2026

August 2026 Composite

October 11, 2026

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Image Details

Lights around Pensacola, Florida, and along the U.S. Route 98 corridor toward Destin appear sharply reduced on October 11, 2026 (right), compared with typical conditions in August 2026 (left), suggesting widespread power outages after Hurricane Isaias. Images are from NASA’s Black Marble HD product.

After a quiet start to the 2026 Atlantic hurricane season, Isaias became the season’s first hurricane on October 8 as it tracked toward the U.S. Gulf Coast. The storm brought heavy rain and flash flooding to parts of the Southeast, including Alabama and the Florida Panhandle, and winds that toppled trees and downed power lines, leaving many people in the dark.

Isaias made landfall near Destin, Florida, on the evening of October 9 as a Category 2 hurricane with maximum sustained winds of 105 miles (170 kilometers) per hour. Gusts topped 100 miles per hour along a corridor west of the storm’s center, according to the National Weather Service, with preliminary reports showing a 117-mile-per-hour gust in Oriole Beach and a 102-mile-per-hour gust at Pensacola City Hall.

These areas of high winds overlapped a broader area west of the storm’s eye where satellite images showed substantial decreases in nighttime lights. The image pair above shows nighttime lights before and after the storm. The left image is a composite of August 2026 data representing typical conditions, and the right image shows lights on October 11, after most of the storm’s clouds had cleared.

The data depicted in the images, provided by Ranjay Shrestha of NASA’s Black Marble science team, come from the Black Marble HD product. The product uses data from the VIIRS (Visible Infrared Imaging Radiometer Suite) on the NOAA-20 satellite, which has a day-night band that detects light emitted and reflected at night. The team processed the data to account for changes in the landscape, the atmosphere, and phase of the Moon, and to filter out stray light that does not come from electric lights. Dark gray, hash-marked areas show where clouds prevented VIIRS from collecting data. The nighttime lights are shown over a base map from the Landsat 9 satellite.

“Standard Black Marble nighttime lights imagery, available through NASA Worldview, provides a broad picture of the storm’s immediate impacts,” Shrestha said. “Black Marble HD takes this a step further by allowing us to visualize these changes at a much finer spatial scale.”

At these finer scales, the images reveal lights decreasing sharply around parts of Pensacola, Florida, and along the U.S. Route 98 corridor toward Destin, suggesting widespread power disruptions. Shrestha also pointed out pockets where lights persisted, including Pensacola International Airport, Pensacola Christian College, and parts of downtown Pensacola. “These patterns could reflect backup power systems, differences in electrical infrastructure, or areas that maintained electricity during the storm, although the imagery alone cannot confirm the underlying reasons,” he said.

October 11, 2026

October 12, 2026

October 11, 2026October 12, 2026

October 11, 2026

October 12, 2026

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Image Details

Widespread outages darken the region around Pensacola, Florida, and along the U.S. Route 98 corridor toward Destin on October 11, 2026 (left). By October 12 (right), lights have returned to some affected areas. Images are from NASA’s Black Marble HD product.

Black Marble HD images also reveal the pace and spatial patterns of recovery. The image pair above compares the same October 11 view (left) with one from October 12 (right), when lights had begun to return to some affected areas. By October 14, lighting patterns looked similar to pre-storm conditions.
 
“Understanding where recovery is progressing and where disruptions persist can help emergency responders and decision makers identify areas that may require additional attention, prioritize resources, and assess the effectiveness of restoration efforts,” Shrestha said.
 
Black Marble data complement ground-based outage reports rather than replace them, offering a more comprehensive view of disasters’ impacts and recovery. “Ultimately, this is where the value of Black Marble lies: turning nighttime Earth observations into actionable insights that support informed decisions and help bridge the gap between Earth science and action,” Shrestha said.
 
The NASA Disasters Program, in coordination with FEMA and the USGS Coastal Storms Team, is supporting the Alabama Red Cross and the Alabama Emergency Management Agency’s response to Hurricane Isaias. The team will be posting maps and data products on its open-access mapping portal as new information becomes available.

NASA Earth Observatory images by Lauren Dauphin, using Black Marble HD data courtesy of Ranjay Shrestha/NASA’s Goddard Space Flight Center and Landsat data from the U.S. Geological Survey. Story by Kathryn Hansen.

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References & Resources

• NASA Disasters Program (2026, October 8) Black Marble HD. Accessed October 15, 2026.
• National Hurricane Center (2026, October 11) Hurricane ISAIAS Advisory Archive. Accessed October 15, 2026.
• National Public Radio (2026, October 11) Hurricane Isaias: By the numbers. Accessed October 15, 2026.

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Shortly after NASA’s Artemis II mission splashed down on April 10, 2026, U.S. Navy divers captured underwater imagery of the Orion spacecraft’s heat shield. In the months after, the agency measured whether the thermal protection system effectively safeguarded the crew and Orion systems as the spacecraft reentered Earth’s atmosphere. This rigorous analysis confirmed that the heat shield performed as expected.

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NASA’s Artemis II mission sent four astronauts around the Moon and brought them safely back to Earth, laying a foundation for crewed flights to the Moon’s surface.

Additional engineering data analysis of the Orion spacecraft’s heat shield confirmed initial data showing the heat shield performed as expected.  

In particular, NASA measured whether the thermal protection system effectively safeguarded the crew and Orion systems as the spacecraft reentered Earth’s atmosphere. This test flight was the first time astronauts flew aboard Orion. 

Orion reached a maximum velocity of 39 times the speed of sound and experienced external temperatures exceeding 4,000 degrees Fahrenheit at its peak, all while the four astronauts inside Orion stayed relatively cool with a cabin temperature in the mid-70 degree Fahrenheit range during their return to Earth from the Moon.  

After NASA’s thorough analysis of Artemis I heat shield findings, informed by extensive arc jet material testing at NASA’s Ames Research Center in California’s Silicon Valley, the agency modified Orion’s reentry trajectory for Artemis II by shortening the maximum downrange distance the spacecraft could fly between when it entered Earth’s atmosphere and splashed down in the Pacific Ocean. Analysis prior to the mission showed that limiting downrange distance would limit how long the spacecraft’s heat shield spent in the temperature range at which the Artemis I heat shield phenomenon occurred.  

The spacecraft reentered with precision, entering within only 192 feet of its targeted entry interface, and successfully splashed down only 0.59 miles from the predicted landing site off the coast of San Diego. Initial inspections of the thermal protection system, including diver imagery of the spacecraft’s heat shield taken just after splashdown and further inspections on the recovery ship, found it performed as expected, with a significant reduction in the amount of cracks and char loss as compared to Artemis I.  

Upon the spacecraft’s return to NASA’s Kennedy Space Center in Florida after the Moon mission, thermal protection system experts began additional examination of the heat shield, made of 186 unique blocks of an ablative material called Avcoat. The heat shield was then transported to NASA’s Marshall Space Flight Center in Huntsville, Alabama, where work on sample extraction and internal x-ray scans began in August to provide further engineering insight into the system and behavior of the material.

A thorough post-flight assessment review found that Orion’s aerodynamic and aerothermal performance, including the heat shield and backshell thermal protection system, was in line with engineering predictions based on pre-flight analyses and ground testing. The shorter allowable down range during entry reduced the cracking and char loss experienced on the Artemis II heat shield relative to the Artemis I heat shield by a factor of ten, proving the effectiveness of the trajectory modification. Engineers found only nine spots of char loss of varying sizes on the Artemis II heat shield dish, compared to 103 during Artemis I. 

The analysis also showed that Orion’s robust heat shield design showed consistency from Artemis I to Artemis II, evident by the performance of system features such as the seams between the heat shield Avcoat blocks and the Avcoat surrounding the heat shield compression pad separation bolts. 

Post-flight inspection of Orion’s backshell, the protective cover on the sloped sides of the crew module made up of 1,300 ceramic tiles, showed expected performance across the crew module surface. Visual inspections indicated backshell features designed to seal and protect penetrations such as windows, vents, thrusters, and the side hatch also met expectations, with no signs of overheating observed. 

The team also performed post-flight laser scans of the heat shield surface and is comparing this data to pre-flight measurements to determine material recession, which will then be compared to analysis predictions. Engineers are continuing with heat shield sample extraction at NASA Marshall and subsequent material test and assessment and thermal analysis, to support long-term heat shield development, manufacturing efforts, and data capture. 

Orion’s performance and the team’s analysis on Artemis II reflect system robustness, capability to support crew, and critical insights gathered that will enhance the Artemis III mission and beyond. Following the extensive Artemis I heat shield investigation, upgrades were made to the heat shield design for Artemis III to achieve uniformity and consistent permeability of the Avcoat blocks. Technicians attached the heat shield for the Artemis III Orion crew module at NASA Kennedy in early July, and the Orion crew and service modules were joined at the end of July. The spacecraft has since been successfully powered up for the first time, enabling engineers to check all connection lines between the two modules are working as planned.

NASA continues to advance toward Artemis III as teams ready the Orion spacecraft for next year’s mission in low Earth orbit. NASA will launch the SLS (Space Launch System) rocket and Orion spacecraft with NASA astronauts Randy Bresnik, Frank Rubio, Andre Douglas, and ESA (European Space Agency) Luca Parmitano, to rendezvous with human lander test articles from Blue Origin and SpaceX to demonstrate critical systems and operations needed for future lunar landings, beginning with Artemis IV in 2028.

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