Rigorous Analysis Confirms NASA’s Artemis II Heat Shield Performance 

A post‑mission comparison of the Orion spacecraft heat shields from Artemis I (left) and Artemis II (right) are shown after removal from their crew modules. Both heat shields are seen rotated for inspection inside the Operations and Checkout Building at NASA’s Kennedy Space Center in Florida.
NASA

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.  

Shortly after Artemis II splashdown on April 10, 2026, U.S. Navy divers captured underwater imagery of the Orion spacecraft’s heat shield.
US Navy

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.

The Artemis II Orion crew module after being offloaded from the well deck of USS John P. Murtha at Naval Base San Diego and lifted from the Orion Recovery Cradle Assembly on April 18, 2026. The gray area, as seen on the edge where the spacecraft’s heat shield and the backshell meet, is from recovery operations.
NASA/Kevin Davis

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. 

The Artemis II Orion crew module is lifted from its recovery fixture for inspection and engineering imagery after being offloaded from the USS John P. Murtha at Naval Base San Diego on April 18, 2026. The recessed areas, or smaller concentric circles, seen on the heat shield are associated with the separation bolts that connect the crew module with the service module. The larger circular patterns are formed due to compression pad material used within this location of the spacecraft, creating flow disturbances caused by extreme aerodynamic and thermal airflow during reentry. This causes increased heating locally and therefore Avcoat ablator thickness is increased in these areas by design.
NASA/Kevin Davis

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.

A person lies on the floor of a workshop, holding a flashlight to inspect the underside of a large, circular heat-shield-like structure suspended above them. The individual is positioned on their side beneath the hardware, with tools and equipment visible in the background.
An engineer from NASA’s Ames Research Center inspects the Artemis II Orion heat shield at NASA Kennedy’s Multi-Purpose Payload Facility on April 30, 2026, prior to its removal from the crew module. The orange tint seen between Avcoat tiles is an expected effect of the silicone used to fill the gaps between the blocks. The silicone gap filler contains iron oxide, which gives it a red appearance after enduring reentry. 
NASA/Kevin Davis

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.

Source: www.nasa.gov

Chandra Finds Possible Origin of ‘Treble Clef’ Waves

A composite image of a remarkable radio wave formation that strongly resembles a treble clef musical symbol, hovering in the midst of two colliding galaxy clusters. Here, galaxies in the galaxy clusters, plus foreground and background stars and galaxies, blanket the image with specks of light set against the blackness of space. At the center of the frame is a large, oval, blue-purple cloud with ragged edges. In the middle of the purple field, tilting slightly to our left, is what appears to be a giant treble clef, loosely drawn with a neon pink marker. Like the musical notation for which it's named, the formation has a strong vertical stroke with a continuous, fluid line swooping back and forth as it moves from top to bottom.
X-ray: NASA/CXC/INAF-IRA/A. Botteon et al.; Infrared: UKIDSS-GPS ; Radio: ASTRON/LOFAR; Image processing: NASA/CXC/SAO/N. Wolk

A formation of radio waves looks remarkably like a treble clef in this Oct. 14, 2026, image from NASA’s Chandra X-Ray Observatory. Researchers used Chandra to find that the Treble Clef is likely caused by an outburst from a supermassive black hole, followed by a collision of two galaxy clusters.

Read more about this discovery.

Image credit: X-ray: NASA/CXC/INAF-IRA/A. Botteon et al.; Infrared: UKIDSS-GPS ; Radio: ASTRON/LOFAR; Image processing: NASA/CXC/SAO/N. Wolk

Source: www.nasa.gov

APOD: 2026 October 15 – The Milky Way over Manhattan

APOD

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

A black and white view of the Manhattan skyline merges into a night sky with stars and a visible, though faint, Milky Way. Please see explanation for more details.

The Milky Way over Manhattan

Explanation: The city lights outshine the stars in the City That Never Sleeps. Who would have thought that the Milky Way could be visible in this sky? This image was taken with a filter that blocks most visible light, capturing instead only light in the near-infrared region of the electromagnetic spectrum (with lower energy than visible light). The astrophotographer’s clever setup blocks most of the light pollution from the city: old incandescent light bulbs and some neon lights are still bright in the near-infrared, but fluorescent and LED light bulbs are not. Of course, stars are also bright in the near-infrared! This image is a reminder that we all live under the same sky, and astronomy allows all of us to learn more about humanity’s place in the Cosmos.

Tomorrow’s picture: Chasing the ISS

Date October 15, 2026
Credit & Copyright Jason Kurth, Ty Buckley
Authors & editors: Cecilia Chirenti, Robert Nemiroff, Jerry Bonnell, Keighley Rockcliffe
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

Source: science.nasa.gov

Fires Arrive in the Amazon Rainforest

Thick gray smoke partially obscures the Amazon River and surrounding rainforest near the cities of Manaus and Santarém. Puffy white clouds rise above the smoke on the left side of the image.

Unlike a tornado or thunderstorm that can deliver destruction in minutes, El Niño exerts its influence over many months. This year, a drought accompanying El Niño has left the Amazon rainforest primed to burn, and scientists say the region has entered the early stages of what they think will be a long and severe fire season.

Starting in September 2026, satellites detected sharp increases in fire activity and smoke emissions in the central and eastern Amazon, visible in fire and emissions monitoring platforms including NASA’s Fire Information for Resource Management System (FIRMS), the Global Fire Emissions Database (GFED), and NASA Worldview. The region with elevated fire activity stretches from forests surrounding the commercial and transportation centers of Manaus and Santarém to the mouth of the Amazon River.

When the MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Aqua satellite captured this image of smoke streaming from fires on both sides of the Amazon River on October 12, 2026, heavy smoke socked in Manaus, the capital of the Brazilian state of Amazonas. That day, city officials reported extremely poor air quality, with fine particulate matter (PM2.5) values above 135 micrograms per cubic meter, the second-worst rating on a regional air quality index. The pall disrupted daily life in a city of more than 2 million people. Schools closed, and citywide events and children’s sports leagues were canceled as officials warned of hazardous air quality, according to news reports.

The burning around Santarém and Manaus is part of a “cascade” of fire in the tropics that accompanies the disrupted rainfall patterns of an El Niño, said Douglas Morton, an Earth system scientist based at NASA’s Goddard Space Flight Center. The pattern begins along the equator with drought and peat fires in Indonesia, followed by elevated fire activity in this part of the Amazon. Morton and colleagues from the University of California, Irvine; Vrije Universiteit Amsterdam; and the University of Maryland detailed the pattern in a 2017 study following the destructive fire season that accompanied the 2015–2016 El Niño. They also saw the pattern play out in 2023.

A swell of fire in the tropics riding the 2026 El Niño has followed the pattern. Drought, fire, and smoke have smothered parts of Indonesia since August, with hundreds of homes razed in October and thick smoke blanketing whole islands most days. “Now, in the Amazon, we’re seeing the second domino in the cascade fall,” Morton said, referring to the uptick in fires that has begun in Pará and Amazonas.

Morton and his colleagues expect the next wave of fire to hit farther north in November and December in the Brazilian states of Roraima, northern Pará, and Amapá, as well as parts of Venezuela, Guyana, and Suriname. Finally, around August and September 2027, he said, drought and fire risk will peak in the southern Amazon regions of Brazil and Paraguay.

“It’s so striking—and frustrating—that this is happening all over again,” said Morton, adding that many of the same forests that burned during the El Niño events in 2023 and 2015 are burning again. Forest fires in these rainforests are known to cause especially serious ecological damage because most species are not adapted to fire. It’s likely that some of the forest fires will burn even more intensely this time because the earlier fires partially charred trees, degrading the forest and making what remained more susceptible to burning, he added.

Morton expects the fires around Santarém and Manaus to continue burning until the rainy season arrives in December 2026 or January 2027. For the regions to the north and south, there is still time to prepare. “Given the intensity of this El Niño, this really is the year for people to avoid burning at all costs,” Morton said.

It’s so wet in the Brazilian Amazon that lightning ignites less than 1 percent of fires, so the vast majority of fires currently burning there were started by people, Morton said. But this year’s drought, worsened by El Niño, has been intense. Brazil’s National Institute of Meteorology reported that Manaus rainfall levels were 95 percent less than normal in August and 60 percent less than normal in September.

The large fires in this region began as management fires—clearing shrubs from pastures or crops from fields, for instance—but have escaped and are now burning freely through the parched understory of the rainforest, he added. Analysis of satellite observations indicates there are 50 to 70 uncontrolled fires burning in the Santarém region alone, said Shane Coffield, a University of Maryland assistant research scientist at NASA Goddard.

As part of a NASA Earth Action project, Coffield is mining fire observations from VIIRS (Visible Infrared Imaging Radiometer Suite) to identify fires that didn’t meet the threshold for inclusion in official data products distributed by FIRMS. He plans to share the locations of these “candidate fires” with scientists at MapBiomas, a multi-institutional network comprising universities, NGOs, and technology companies that maps fires and land-use change in the Amazon.

“For the area around Santarém, we’ve identified about 40 percent more fires than you’ll see in active fire counts from FIRMS,” said Coffield. Satellites often miss fires in circumstances like this due to dense smoke, clouds, and tree canopy cover, which can block the sensors from detecting the infrared signal of fires—especially lower-intensity fires spreading along the forest understory. “On some of the smokiest days, we have very few detections from MODIS and VIIRS, and we know that isn’t right.”

NASA Earth Observatory images by Lauren Dauphin, using MODIS data from NASA EOSDIS LANCE and GIBS/Worldview. Story by Adam Voiland.

References & Resources

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Peatland Fires Darken Skies in Indonesia

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Source: science.nasa.gov

NASA to Host News Conference Previewing US Spacewalks 100, 101

NASA astronaut and Expedition 75 flight engineer Anil Menon conducts a spacewalk to prepare the International Space Station for future upgrades to its power system. Menon helped build a modification kit on the station’s Starboard 6 truss segment where a roll out solar array is slated to be installed later this year.
NASA astronaut Anil Menon conducts a spacewalk on Aug. 6, 2026, to prepare the International Space Station for future upgrades to its power system.
Credit: NASA

NASA will preview two upcoming spacewalks to complete solar array installation and power augmentation of the International Space Station during a news conference at 2 p.m. EDT, Tuesday, Oct. 20, from NASA’s Johnson Space Center in Houston.

NASA will stream the event through a variety of platforms. Learn where to watch online:

https://www.nasa.gov/live

NASA participants in the news conference include:

  • Gaurang Patel, operations integration manager, Low Earth Orbit Program
  • Garrett Hehn, spacewalk flight director, Flight Operations Directorate

United States-based media interested in attending in person must contact the Johnson newsroom no later than 3 p.m., Monday, Oct. 19, at: [email protected]. Media joining by phone should request dial-in details by the same deadline. To ask a question, media must dial in no later than 15 minutes before the start of the news conference.

Thursday, Oct. 29

During U.S. spacewalk 100, NASA astronaut Anil Menon and CSA (Canadian Space Agency) astronaut Joshua Kutryk will exit the station’s Quest airlock to install and deploy an International Space Station Roll-Out Solar Array (IROSA) on the 2A electrical power channel. The solar array will be the seventh IROSA and will provide additional power to support critical station operations, including its safe and controlled deorbit.

Thursday, Nov. 5

During U.S. spacewalk 101, Menon and Kutryk will install and deploy the eighth and final IROSA on the 3B channel of the space station, completing the power augmentation upgrades.

The final two roll-out solar arrays will complete the space station’s power system augmentation. Together, the eight roll-out arrays will increase available power by up to 30%, boosting the station’s electric power generation capacity from 160 kilowatts to approximately 215 kilowatts.

NASA will share additional coverage details about U.S. spacewalks 100 and 101 closer to each operation on the agency’s live events web page and the space station blog. The spacewalks will be the 285th and 286th conducted in support of space station assembly, maintenance, and upgrades.

To learn more about International Space Station research, operations, and its crews, visit:

https://www.nasa.gov/station

-end-

Joshua Finch / Jimi Russell
Headquarters, Washington
202-358-1100
[email protected] / [email protected]

Sandra Jones / Anna Schneider
Johnson Space Center, Houston
281-483-5111
[email protected] / [email protected]

Source: www.nasa.gov

An Impact Structure With Legs

Several short, light-colored rocky ridges radiate out from a central point amid an orange and tan desert landscape.

Editor’s Note: Today’s story is the answer to the October Puzzler.

From above, the mere appearance of a curious geologic feature in Western Australia is enough to cause a fright. The aptly named Spider Crater, the product of a meteorite impact followed by hundreds of millions of years of erosion, sprawls across the landscape in the country’s Kimberley region.

The OLI (Operational Land Imager) on the NASA-USGS Landsat 9 satellite captured this image of the crater on September 20, 2026. The full impact structure has an oval shape measuring about 13 kilometers by 11 kilometers (8 miles by 7 miles), with the spiderlike central portion measuring about 4 kilometers (2.5 miles) across.

Geologists believe the unusual arachnoid pattern is the remnant of a central uplift, the raised portion of the crater floor that formed in the rebound of the initial impact shock. The light-colored “legs” are sandstone ridges that have endured while other rock layers in the impact zone have eroded away.

For decades after the feature’s discovery, scientists struggled to weave a tale about its formation. Some proposed it had a volcanic past. But with some legwork in the field, geologists identified telltale signs of a past impact: fan-shaped fractures called shatter cones. These fractures form only when intense shock waves travel through rock, and they are ubiquitous in Spider Crater’s central dome.

Scientists have subsequently performed lab analyses of shocked quartz and zircon crystals from the sandstone, which can help them reconstruct the angle of the meteorite’s impact. The date of the impact is uncertain, but estimates based on rocks in the region place it between about 900 million and 600 million years ago—making Spider Crater a creature of the late Precambrian.

NASA Earth Observatory image by Michala Garrison, using Landsat data from the U.S. Geological Survey. Story by Lindsey Doermann.

References & Resources

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Source: science.nasa.gov

NASA’s Chandra Breaks Down ‘Treble Clef’s’ Galaxy Cluster Collision

Using Chandra, astronomers have discovered that an outburst from a supermassive black hole, followed by a collision of two galaxy clusters, are the likely causes of an unusual formation in a galaxy cluster. The “Treble Clef” radio source was given its nickname because of a distinct shape in radio waves that resembles the musical symbol. This composite image of the Treble Clef and its galaxy cluster contains X-rays from Chandra and eROSITA, radio data from LOFAR, and infrared data from UKIRT.
X-ray: NASA/CXC/INAF-IRA/A. Botteon et al.; Infrared: UKIDSS-GPS ; Radio: ASTRON/LOFAR; Image processing: NASA/CXC/SAO/N. Wolk

Astronomers have used NASA’s Chandra X-ray Observatory to break down the cause of a remarkable formation of radio waves they have nicknamed the “Treble Clef” because its distinct shape strongly resembles the musical symbol.

The researchers discovered the Treble Clef is likely caused by an outburst from a supermassive black hole, followed by a collision of two galaxy clusters. A paper describing the findings, led by Andrea Botteon of the National Institute for Astrophysics, or INAF, in Italy, published Wednesday in the Astronomy & Astrophysics journal.

An explanation for the Treble Clef has been particularly difficult to find because the formation lies almost directly behind the plane of the Milky Way, meaning that stars, gas, and dust from our home galaxy largely block the view from Earth. However, by using telescopes that can peer through the intervening material, a team of researchers was able to identify what is responsible for this uncommon structure.

NASA’s Chandra and the German Extended RÖntgen Survey with an Imaging Telescope Array (eROSITA) X-ray telescope found diffuse, hot gas at the location of the Treble Clef, showing that a galaxy cluster hosts the object. The researchers also determined the galaxy cluster is, in fact, two clusters in the process of merging. Galaxy clusters are some of the largest structures in the universe, containing hundreds of individual galaxies and huge reservoirs of superheated gas.

This new composite image of the Treble Clef and its cluster shows the multimillion-degree gas detected in X-rays by Chandra and eROSITA in blue, with some of the Chandra data derived from a special technique the authors used to highlight important features in the Chandra data. Radio data shown in red from the LOw Frequency ARray (LOFAR), a large network of radio telescopes in Europe reveals the doppelganger of the musical notation. The final piece of the combined image comes from infrared data obtained by the United Kingdom Infrared Telescope, appearing mostly white.

The authors concluded that the Treble Clef likely formed in a two-stage process. First, an earlier outburst from a supermassive black hole in the galaxy cluster’s center drove clouds of charged particles and magnetic fields away at close to the speed of light. This led to a type of cosmic crescendo and initially produced bright radio waves that later faded as the particles lost energy. Next, the collision between the two clusters compressed or reenergized the cloud, which became brighter again in radio waves. Shock waves — similar to the sonic booms from supersonic jets — from the collision may have played a role in this reenergizing process.

To reveal evidence for the cluster collision in the Chandra data, the authors used a special technique that examined how much the cluster’s hot gas deviates from a symmetrical shape. Most of the hot gas is symmetrical and shaped approximately like an oval. The authors removed this symmetrical oval shape from the original X-ray image. The remaining X-ray emission in the residual image shows t is brightest on the left and right, and faintest in the center. The new composite image combines both the original X-ray and the residual X-ray images.

The brighter X-rays in the residual image, toward the left and right of the cluster’s center, imply that the collision between the two clusters likely occurred along the left-right direction as seen in the image. The researchers think the direct collision between the two clusters occurred a few hundred million years ago, and the clusters are now moving away from each other.

The resemblance to a treble clef is a case of pareidolia, the phenomenon when people see familiar shapes in random data, since there is no scientific connection to the musical notation.

NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.

To learn more about Chandra, visit:

https://nasa.gov/chandra

Visual Description

This release features a composite image of a remarkable radio wave formation that strongly resembles a treble clef musical symbol, hovering in the midst of two colliding galaxy clusters.

Here, galaxies in the galaxy clusters, plus foreground and background stars and galaxies, blanket the image with specks of light set against the blackness of space. At the center of the frame is a large, oval, blue-purple cloud with ragged edges. This is a multimillion-degree gas cloud in the two clusters detected in X-rays by Chandra and eROSITA, the Extended RÖntgen Survey with an Imaging Telescope Array.

In the middle of the purple field, tilting slightly to our left, is what appears to be a giant treble clef, loosely drawn with a neon pink marker. Like the musical notation for which it’s named, the formation has a strong vertical stroke with a continuous, fluid line swooping back and forth as it moves from top to bottom.

This radio wave formation appears to be the result of a two-stage process. First, charged particles and magnetic fields were driven from a supermassive black hole, producing bright radio waves. Those waves faded and lost energy over time, before being reenergized and compressed when the two galaxy clusters collided.

Details

Last Updated

Oct 14, 2026

Editor
Lee Mohon
Contact
Megan Watzke
Joel Wallace
Location
Marshall Space Flight Center

Source: science.nasa.gov

NASA’s Space X CRS-35 Launch Jellyfish

The exhaust plumes of a SpaceX Falcon 9 rocket carrying the company’s Dragon spacecraft are seen illuminated by sunlight against the predawn sky.
NASA/John Kraus

Sunlight illuminates the exhaust plumes of a SpaceX Falcon 9 rocket carrying the company’s Dragon spacecraft on Oct. 13, 2026. This visual phenomenon is known as a “jellyfish”; it happens near sunrise or sunset when the exhaust plume from the rocket becomes brightly illuminated, creating a glowing shape resembling a jellyfish.

The mission lifted off at 6:33 a.m. EDT from Space Launch Complex 40 at Cape Canaveral Space Force Station, carrying scientific investigations, supplies, and equipment to the International Space Station on SpaceX’s 35th commercial resupply services mission for NASA. The rocket’s exhaust plumes were visible across the eastern United States.

Watch the uncrewed Dragon spacecraft rendezvous with and dock to the International Space Station on Oct. 15. Coverage begins at 9:15 a.m. EDT.

Image credit: NASA/John Kraus

Source: www.nasa.gov

NASA Develops Batteries to Power Humanity’s Return to Moon

5 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

Yi Lin, SPEARS testing and research lead at NASA Langley, holds one of the small coin-cell batteries that had just undergone thermal vacuum testing.
Yi Lin, SPEARS testing and research lead at NASA Langley, holds one of the small coin-cell batteries that had just undergone thermal vacuum testing.
NASA/Ryan Hill

If you’ve ever had your car start sluggishly, or not at all, on a particularly frigid winter morning, you know standard batteries do not like extreme cold. That’s why NASA researchers are working to develop a battery that could function in the brutal cold of the Moon’s South Pole, where nighttime temperatures plunge to minus 328 degrees Fahrenheit (minus 200 Celsius). 

For future lunar operations, a battery will need to work immediately when warmed up and be able to power everything from an astronaut’s emergency kit to a rover capable of exploring the Moon’s darkest craters — all without posing a fire hazard. 

A team of NASA researchers is working to make all that happen. The project is called Solid Power for Extreme Environment Adaptability and Resilience in Space (SPEARS), and it could provide NASA with an important tool to help power humanity’s sustained presence on the Moon through the Artemis campaign. 

“Batteries have become an important part of our lives here on Earth, which enable our laptops, cell phones, power tools, and even our vehicles,” said Donald Dornbusch, principal investigator for SPEARS at NASA’s Glenn Research Center in Cleveland, where the project is led. “We will need them on the Moon, too, and these batteries will be required to operate reliably and safely in this harsh environment. That’s why we’re working on this technology.” 

Yi Lin, left, SPEARS testing and research lead, and Ji Su, a polymer materials scientist and the task lead, during the removal of SPEARS batteries from thermal vacuum testing at NASA Langley.
Yi Lin, left, SPEARS testing and research lead, and Ji Su, a polymer materials scientist and the task lead, during the removal of SPEARS batteries from thermal vacuum testing at NASA Langley.
NASA/Ryan Hill

Splashy problem, solid solution

Traditional lithium-ion batteries like those in your cell phone and laptop have a critical weakness: they rely on liquid electrolytes. Cool a conventional battery to the Moon’s nighttime temperatures, and that liquid would freeze, potentially damaging the battery. Heat it up too much — say, to daytime lunar temperatures of 212 F (100 C) — and it won’t work until cooled. Expose the liquid to the vacuum of space, and it evaporates. 

SPEARS batteries solve these problems by replacing the liquid electrolyte with a solid ceramic- or polymer-based material. This change could unlock several advantages. First and foremost, they could operate in the heat and extreme cold. 

During recent thermal vacuum testing at NASA’s Langley Research Center in Hampton, Virginia, small prototype battery cells operated well up to 176 F (80 C), down to minus 76 F (minus 60 C), and with slightly reduced performance down to minus 112 F (minus 80 C). 

“We proved for the first time that these cells can work down to minus 80 degrees Celsius,” said Yi Lin, SPEARS testing and research lead at NASA Langley.  

Lin also said he’s confident they can improve performance and maybe even expand that range in coming years. 

The batteries need to remain reliable through exposure to the Moon’s wild temperature swings between day and night. The thermal vacuum testing showed that after exposure to temperature extremes from 212 F (100 C) to minus 274 F (minus 170 C), SPEARS batteries don’t sustain damage.  

Just like the chemistry in your earbuds is different from the chemistry in your phone, which is different from the chemistry in your car, all these chemistries can still function with a solid electrolyte. We can tune for energy, tune for power, tune for durability, depending on the application.

Yi Lin

Yi Lin

SPEARS testing and research lead

Not even solid-state batteries will function while they’re at a temperature as low as minus 274 F, but because solid electrolytes don’t freeze like a liquid, the batteries can survive the extreme low temperatures.  

In order to get the batteries working again after exposure to such cold, small heaters come into play. SPEARS batteries wouldn’t need to be kept warm all the time, just warmed up to operational temperature. That could reduce the need for heavy thermal management systems in spacecraft and lunar habitats, allowing for lighter designs, lower costs, and longer mission durations. 

Nike Lin, a support engineer/technician on the thermal vacuum team, holds up a battery.
Nike Lin, a support engineer/technician on the thermal vacuum team, takes weight measurements of batteries following thermal vacuum testing.
NASA/Ryan Hill

Power for Moon, Earth

The applications for these solid-state batteries are nearly limitless, from small tools like drills that must operate in shadowed lunar craters, to rovers and emergency power packs for astronauts. They also could provide power solutions for long-duration scientific instruments. 

“We can tune the chemistry by using different electrode materials,” said Lin. “Just like the chemistry in your earbuds is different from the chemistry in your phone, which is different from the chemistry in your car, all these chemistries can still function with a solid electrolyte. We can tune for energy, tune for power, tune for durability, depending on the application.” 

While SPEARS is designed for space, the technology could be spun off into Earth-based applications. In fact, SPEARS evolved out of a previous battery project Lin and Dornbusch worked on that focused on aeronautic applications. 

From left to right: Donald Dornbusch (NASA Glenn), Godfrey Sauti, Sang-Hyon Chu, Yi Lin (NASA Langley), and Malachi Mooney-Rivkin (NASA Ames), during a round of TVAC testing at NASA Langley.
From left to right: Donald Dornbusch (NASA Glenn), Godfrey Sauti, Sang-Hyon Chu, Yi Lin (NASA Langley), and Malachi Mooney-Rivkin (NASA Ames), during a round of TVAC testing at NASA Langley.
NASA

“The potential market for solid-state batteries is very broad,” said Ji Su, a polymer materials scientist and the task lead at NASA Langley. “Automobiles, cell phones, communication devices, drones — anything that needs a portable power supply.” 

The SPEARS project began in 2026 with funding through the Advanced Research and Technology division within the agency’s Research and Technology Mission Directorate. The project is set to focus on technology development in its first stages before potentially shifting toward commercial collaboration. NASA’s Ames Research Center in California’s Silicon Valley is working to develop flight hardware such as test boards and electronics to help prepare the SPEARS batteries for spaceflight and test them in space environments. 

Source: www.nasa.gov

NASA to Discuss Artemis Acceleration, Status of Upcoming Moon Missions

As the Artemis II crew members 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. The edge of the visible surface of the Moon is called the “lunar limb."
As the Artemis II crew members 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. The edge of the visible surface of the Moon is called the “lunar limb.”
Credit: NASA

NASA will provide an update on its plans to return American astronauts to the surface of the Moon by 2028 at 2 p.m. EDT, Friday, Oct. 23, at the agency’s Kennedy Space Center in Florida.

Learn where to watch online:

https://www.nasa.gov/live

Participants in the briefing include:

  • NASA Administrator Jared Isaacman
  • NASA Associate Administrator Amit Kshatriya
  • Jeremy Parsons, NASA’s Artemis program manager

The update will include details about NASA’s Artemis III mission that will send four astronauts to low Earth orbit next year to test critical systems needed for future lunar landings, and how plans to return American astronauts to the Moon by 2028 are progressing.

U.S. media interested in attending in person must apply online by 12 p.m., Friday, Oct. 16. To ask questions remotely, media must request the dial-in number from the Kennedy newsroom no later than one hour prior to the start of the update by emailing: [email protected]. NASA’s media accreditation policy is online. 

As part of a Golden Age of innovation and exploration, NASA will send Artemis astronauts on increasingly difficult missions near the lunar South Pole to explore more of the Moon than ever before. In addition to providing economic benefits and advancing scientific discovery through its Moon missions, NASA will establish an enduring human presence on the lunar surface and build on the agency’s foundation for the first crewed mission to Mars.

Learn more about Artemis:

https://www.nasa.gov/artemis

-end-

Rachel Kraft
Headquarters, Washington
202-358-1600
[email protected]

Tiffany Fairley
Kennedy Space Center, Fla.
321-867-2468
[email protected]

Details

Last Updated

Oct 14, 2026

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Source: www.nasa.gov