NASA Calls for Proposals to Accelerate Lunar Surface Technologies 

NASA Calls for Proposals to Accelerate Lunar Surface Technologies 

Artistic concept of lunar surface technologies and infrastructure capabilities, including in-situ resource utilization oxygen production systems, surface power systems, in-space manufacturing tools, and advanced nanomaterials production.
Credit: NASA

NASA is seeking proposals to advance the technology and infrastructure needed to explore the Moon and establish a Moon Base in the lunar South Pole region.

Announced on Tuesday, Sept. 8, the solicitation targets capability gaps, including power generation, oxygen extraction, and producing materials on the Moon required for construction and operations. These technologies are essential to making humanity’s next great leap in lunar exploration.

“NASA is accelerating the development of key technologies and closing critical gaps needed for long-term human exploration at the Moon,” said Greg Stover, director of NASA’s Advanced Research and Technology Division. “Partnering with industry will strengthen the U.S. industrial base as we mature the capabilities and infrastructure needed for a sustainable lunar presence.”

The NextSTEP-3 Broad Agency Announcement Appendix A: Lunar Enabling Infrastructure Accelerator solicitation aims to mature and demonstrate capabilities in five areas:

  • Vertical solar array technology that can provide consistent power generation, management, distribution, and energy storage.
  • In-situ resource utilization oxygen from regolith production to extract usable oxygen molecularly bonded to rock and dust covering the Moon’s surface.
  • Radioisotope Stirling generator, a type of nuclear energy technology that uses heat from fissile materials to produce electric power for operating spacecraft systems in the darkest, dustiest, and most remote places.
  • In-space advanced manufacturing to reduce reliance on resupply missions from Earth and to optimize mission flexibility and resilience on the Moon.
  • Innovative nanomaterials production to advance the commercial availability and quality of nanomaterials that can be used in lunar exploration.

The solicitation intends to cultivate U.S.-led capabilities while maintaining full and open competition among private industry, academic institutions, and not‑for‑profit entities, as well as international partners participating through U.S.-led teams. 

NASA may apply insights gained from the resulting contracts of this solicitation, such as technical data, and demonstration results, to shape future acquisition strategies.  

To learn more about NextSTEP-3, visit:

https://go.nasa.gov/4x20o3t

-end-

Rob Margetta
Headquarters, Washington
202-358-0918
robert.j.margetta@nasa.gov

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Sep 08, 2026

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Lauren E. Low

Superbubble in the Large Magellanic Cloud

Superbubble in the Large Magellanic Cloud

Blue and orange stars shine through a wispy bubble of gas; the center is mostly clear, but blue and gray tendrils snake throughout most of the rest of the image. The background of the image is filled with other stars.
NASA, ESA/Hubble, D. Gouliermis

NASA’s Hubble Space Telescope captures a photogenic nebula, N44, in the Large Magellanic Cloud in this Sept. 3, 2026, image. N44 is dominated by two features: a vast central void and a shell of dense, dusty gas. The central void is a ‘superbubble’ spanning roughly 210 by 140 light-years across. The glittering stars at the center of the void are responsible for its creation; through their powerful stellar winds and explosive supernovae, these stars expelled much of the gas from which they were born.

Read more about this cosmic vista.

Image credit: NASA, ESA/Hubble, D. Gouliermis

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NASA Technique for Manipulating Satellite Photos Now Reveals Ancient Images  

NASA Technique for Manipulating Satellite Photos Now Reveals Ancient Images  

3 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

A man stands in front of a rock with art on it, the colors are intense and exaggerated revealing an intricate design in the rock's surface.
Jon Harman poses in front of an example of the Rancho Bernardo style of Native American artwork that’s barely visible until Dstretch is applied. 
Credit: Jon Harman 

High in the central tower in the ancient Cambodian temple of Angkor Wat, paintings depict horseback riders and a traditional musical ensemble. Thousands of visitors pass these images daily without noticing, because they’re faded to the point of invisibility. 

They were discovered between 2010 and 2012, along with about 200 other paintings throughout the complex, by an archaeologist using a method conceived at NASA’s Jet Propulsion Laboratory in Southern California. 

The technique, known as decorrelation stretch, heightens contrasts in digital imagery, making features easier to spot. It is especially popular for studying ancient rock art, partly due to the chance intersection of one man’s hobby with his professional background. 

Around 2005, rock art enthusiast Jon Harman saw NASA images depicting the Martian surface with and without the application of decorrelation stretch. Seeing how much detail the technique revealed, Harman, now retired in Pacifica, California, understood the implication for studying ancient, faded images. 

He also worked in medical imaging. “I Googled it and found a NASA paper that explained how to do the algorithm,” he said. “I knew from my medical imaging experience that I could do it, so I did.” 

The paper was written in 1996 by Ronald Alley, a JPL employee developing applications for the Advanced Spaceborne Thermal Emission and Reflection Radiometer (ASTER), a Japanese imaging instrument on NASA’s Terra satellite. One of Alley’s former supervisors at JPL had coinvented decorrelation stretch, and Alley had recognized its potential for gleaning information from ASTER imagery.  

Harman made his plug-in for use with ImageJ, an open-source program developed by the National Institutes of Health.  




before
after

A wall with a series of faded humanoid figures painted on it.

A new yellow figure emerges from behind the other after the dstretch algorithm is applied

A wall with a series of faded humanoid figures painted on it.
A new yellow figure emerges from behind the other after the dstretch algorithm is applied

before

after

Before and After

Dstretch applied to Cave of San Borjitas in Baja California, Mexico


As Jon Harman was developing the Dstretch plug-in, he applied it to this image from the Cave of San Borjitas in Baja California, Mexico. When the yellow figure appeared in the middle of the picture, he knew he had something useful. Credit: Jon Harman 

He said he fulfills about 200 requests for Dstretch per year. Around 2010, he also created smartphone apps that use a shortcut to mimic decorrelation stretch. The apps have been downloaded thousands of times, and papers have been published describing Dstretch’s usefulness in archaeology. 

It has been used to spot and clarify imagery at ancient sites under a cliff in Norway, in an Egyptian tomb, at a park in Canada, and in many other locations. It has also helped archaeologists find buried remains of ancient Greek buildings and examine tattoos on mummified human remains, among its non-rock-art applications.  

Harman said he was not surprised Dstretch found wide use in the rock art community. “But I’ve been surprised by a lot of the different applications people have found. So that’s been cool.”  

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Andrew Wagner

1,000 Museum Visitors Dive Into NASA Sea Level Science on World Ocean Day

1,000 Museum Visitors Dive Into NASA Sea Level Science on World Ocean Day

3 min read

1,000 Museum Visitors Dive Into NASA Sea Level Science on World Ocean Day

Several people place their hands and forearms on a brightly lit, abstract patterned surface under colorful fluorescent lighting.
Participants reach into an augmented reality sandbox, reshaping the terrain as projected contour lines and colors illustrate topographic features and elevation changes.
University of Georgia Marine Extension and Georgia Sea Grant

More than 1,000 visitors explored NASA sea level science firsthand during World Ocean Day at the University of Georgia Aquarium on Skidaway Island on June 6, 2026. The free event was supported by NASA’s Science Activation program through the Sea Level Education, Awareness, and Literacy (SEAL) project – a national effort that connects NASA sea level rise data with educators and coastal communities, particularly those historically underserved and already experiencing sea level impacts.

SEAL is a partnership between NASA and four NOAA Sea Grant programs working together to expand sea level rise understanding across U.S. coastal regions. By co-developing lesson plans, interactive activities, and place‑based learning experiences, SEAL helps educators engage learners with real NASA observations, models, and projections while strengthening community resilience to climate change.

During World Ocean Day, SEAL partners at Marine Extension and Georgia Sea Grant and the Coastal Equity and Resiliency Hub at Georgia Tech led hands‑on activities that brought sea level science to life. Visitors played the “Tumbling Tower” game, where removing blocks represents different community impacts from rising seas, and made “sea level friendship bracelets” that used colored glass beads to represent observed sea level rise along local coastlines.

The event also marked the debut of a new augmented reality sand box developed through SEAL. Guests shaped sand into coastal landscapes and watched NASA-informed sea level rise projections transform their creations in real time. Participants could experiment with resilience strategies, such as adding dunes or relocating homes, to see how adaptations might help communities prepare for future change.

Educators – formal, informal, home-based, and more – attending the event were able to take home four different SEAL lesson plans designed for both classrooms and informal learning settings. These materials help students explore sea level rise processes, modeling, variation, and impacts through NASA data and interactive STEM activities. SEAL aims to make all lesson plans developed through the project available online, but until then, please email Shannon Matzke to request digital copies.

“World Ocean Day is an annual tradition at the UGA Aquarium,” said Shannon Matzke, Marine Educator and Public Program Coordinator at UGA Marine Extension and Georgia Sea Grant. “With the support of NASA’s Science Activation program, this year’s event was free, which allowed us to reach more people and different audiences than we typically see. Incorporating SEAL activities made the day even more impactful for visitors – many of whom live in coastal communities already experiencing the effects of sea level rise.”

The SEAL project is supported by NASA cooperative agreement award number NNH21ZDA001N-SCIACT and is part of the NASA Science Activation Program portfolio, which connects learners with authentic NASA science experiences through partnerships with educators and community organizations.

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NASA’s Hubble, Webb Find Far-out Solar System Objects ‘Remember’ Past

NASA’s Hubble, Webb Find Far-out Solar System Objects ‘Remember’ Past

5 min read

NASA’s Hubble, Webb Find Far-out Solar System Objects ‘Remember’ Past

An illustration of a roughly spherical, rocky object against a black background speckled with distant, white stars. The object is the color of red clay and is pockmarked with craters and other geological scars. At the bottom left corner of the illustration in gray lettering is the label “Artist’s Concept.”
This artist’s concept depicts a Trans-Neptunian Object, a small, faint, icy body orbiting the Sun beyond the orbit of Neptune. These objects are so small that even with NASA’s Hubble and Webb space telescopes, they appear only as tiny points of light.
Artwork: NASA, ESA, Leah Hustak (STScI)

For the first time, scientists used the joint power of NASA’s Hubble and James Webb Space Telescopes to study some of the most far-flung bodies in our solar system, Trans-Neptunian Objects (TNOs). Some of these are the smallest and faintest ever directly seen. The researchers unexpectedly found fewer small TNOs than they expected, and that the colors of these bodies followed the same relationships as their larger family members.

These objects are typically small, faint, icy bodies orbiting the Sun beyond the orbit of Neptune. Most are more than 100 million times dimmer than objects visible to the unaided eye. In two complementary papers published Tuesday in The Astronomical Journal, teams analyzed the color, composition, and size distribution of 27 newly discovered tiny, dim TNOs. 

This class of small bodies offers the best view into an early stage of planet-building, when a disk of dust and pebbles in orbit around the Sun coalesced into city-sized “planetesimals” — the solid building blocks that clump together to form planets — but had not yet merged into full-sized worlds.  Beyond Neptune, this second stage never happened, leaving behind a frozen population of planetesimals.

In the deepest TNO survey to date, teams led by PhD candidates from the University of Victoria in Canada, under the guidance of the National Research Council of Canada, and Northern Arizona University in Flagstaff examined a patch of sky simultaneously with Hubble, observing the TNOs’ visible light, and Webb, observing their infrared light. The team of researchers measured the objects’ colors, which are like a fingerprint of the surface composition, as well as their sizes and determined their orbits. 

In the coordinated observations, the teams studied two different types of TNOs. The first, dynamically “cold” TNOs, are on their original, relatively circular orbits around the Sun in the plane of the solar system. The second type, dynamically “hot” TNOs, formed between the current locations of Uranus and Neptune but were pushed outward where they are today when the outer gas giants migrated early in the solar system’s history. Today they reside in highly elliptical orbits and move in and out of the plane of our solar system.

NASA’s Goddard Space Flight Center; Lead Producer: Paul Morris

Prior to these observations, astronomers thought that small TNOs from both hot and cold populations would have undergone many collisions, changing their surfaces compared to larger TNOs. But that’s not what the observations showed. Instead, the small bodies look like their larger counterparts. This implies that collisions are not changing the surfaces significantly—perhaps because there are fewer collisions than expected, or because the TNOs somehow retain their primordial, pre-collision compositions. The teams are still trying to unravel this mystery.

“You could imagine a scenario where getting knocked around and fragmented would change the surface composition, and then you would see a different surface color for tiny TNOs compared to their larger siblings. So it’s really fascinating to see that the smallest objects are somehow ‘remembering’ and preserving the history of how they were made,” said Northern Arizona University PhD candidate Anastasia Morgan, who led the study of color and composition. 

“These dynamically ‘hot’ TNOs retain a signature of where they were born, even though they’ve been orbitally scrambled since then,” said co-author David Trilling of Northern Arizona University.

Both the “hot” and “cold” populations seem to keep the same colors as when they were formed, with little change since the birth of the solar system. 

The Webb data also allowed researchers to measure the number of objects of each size. They found that the overall size distributions for both populations were surprisingly similar.

“It’s very interesting that the process of planetesimal formation ends up producing the same distribution of sizes for both cold and hot populations, despite forming in different regions of the early solar system. The process seems to be insensitive to disk conditions, producing similar planetesimal sizes whether the disk is hot or cold, and dense or fluffy,” said University of Victoria PhD candidate Marielle Eduardo, who led the study on size distribution. 

Researchers also found fewer of these very small bodies than they expected based on some planet formation models. Webb discovered 27 new, remarkably dim TNOs, one so faint it is equivalent to standing on Earth and seeing a small swarm of fireflies on the Moon. The smallest one they observed has a diameter of about 3 miles (5 kilometers), which is about five times smaller than what is possible to detect with the most sensitive ground-based telescopes.

This project would not have been possible without Hubble and Webb working together to detect and characterize these TNOs. With Hubble’s sensitivity in visible light and Webb’s in infrared, the space telescopes provide more insights than either can on its own.

The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.

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

To learn more about NASA’s space telescopes, visit:
https://science.nasa.gov/universe

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Last Updated
Sep 08, 2026
Editor
Andrea Gianopoulos
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov

Ann Jenkins, Christine Pulliam
Space Telescope Science Institute
Baltimore, Maryland

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