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Data from NASA’s Chandra X-ray Observatory, NASA’s James Webb Space Telescope, and NASA’s Hubble Space Telescope combine to reveal a vibrant view of 30 Doradus, or the Tarantula Nebula, in this Aug. 11, 2026, image. Located in the Large Magellanic Cloud, a small neighbor galaxy to the Milky Way about 160,000 light-years from Earth, the Tarantula has thousands of young stars embedded in a vibrant honeycomb-like structure of gas and dust.

By studying the data from Chandra, Hubble, and Webb, combined with data from the agency’s retired Spitzer Space Telescope, astronomers determined that the Tarantula may be losing energy from several sources, including hot gas escaping from the nebula.

Learn more about this image.

Image credit: X-ray: NASA/CXC/Ohio State Univ./J. Rodriguez et al; Infrared: NASA/ESA/CSA/STScI; Optical: NASA/ESA/STScI; Image Processing: NASA/CXC/SAO/P. Edmonds

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NASA Challenge Tests Wheel Designs for Moon Base Mobility

As NASA prepares to establish the Moon Base, advancing surface mobility will be key to helping crews and robotic systems travel farther across the lunar surface. 

To help advance that capability, the Rock and Roll with NASA Challenge invited public innovators to design and build next-generation lunar rover wheels. 

Five teams from 128 submissions and 49 countries advanced to the final phase of the competition, where they tested their prototypes on July 31 at NASA’s Johnson Space Center in Houston. 

The challenge sought lightweight, durable, and scalable wheels that could support longer-duration lunar surface operations. The designs also needed to be compliant enough to absorb impacts, maintain traction at higher speeds, and withstand the harsh lunar environment. 

“Every additional kilometer a rover can reliably travel will expand how far we can explore, what science we can achieve, and what infrastructure we can build,” said Ed Herrera, robotics engineer at Johnson and co-leader of the challenge project. 

NASA Johnson uses ground prototypes to test mobility technologies, while lunar terrain vehicles will be delivered to the lunar surface through the Commercial Lunar Payload Services initiative. For the challenge, the wheels were fitted to MicroChariot, a 45-kilogram test rover, and put through a series of courses at Johnson’s Rock Yard to evaluate their performance across different types of terrain. 

“Crowdsourcing gives us an opportunity to look beyond traditional approaches for lunar wheel design,” Herrera said. “The more wheel technologies we can develop and understand, the more options we have to meet the needs of different vehicles, terrains, and missions on the Moon and Mars.” 

Those ideas were reflected in five distinctly different designs. 

The HTR Variable Flex Lunar Wheel created by Hellenic Technology of Robotics SA uses an internal system designed to vary the wheel’s stiffness depending on terrain and vehicle needs. The team adapted technology it had been developing for terrestrial wheels for about a decade. 

The Hiper Wheel created by Hyperbola uses tensioned cables and a corigated structure that provides spring-like behavior, allowing the wheel to flex without relying on traditional radial spokes. 

The Huff Helo Flexible Titanium Wheel created by Huff Helo Inc. uses formed titanium sheet metal as both structure and spring. During testing, the team found that the strength of the design also made the wheel more rigid, causing it to bounce over some obstacles rather than conform to the terrain. 

The Payne Aviation Wheel created by Deborah and Craige Payne took inspiration from aviation and history. Its designer, an aircraft mechanic, combined a pneumatic approach with ideas from early automobile tire designs. 

The winning Scotch Pad Tyres concept came from an Australian mechanical engineer Daniel Bloomfield and his son Isaac Bloomfield. Their prototype uses a Nomex-based tire structure supported around an aluminum hub. The soft material allows the tire to deform around terrain, while internal support helps it maintain its shape. A treated outer surface of epoxy and corundum grit was integrated to improve traction. 

The Rock Yard testing also demonstrated why different terrains may require different approaches. Loose material can affect traction, while rocks and slopes place different demands on wheels such as vehicle stability. 

As lunar exploration expands, different vehicles will require different combinations of speed, load capacity, durability, and terrain performance. 

Seeking that variety was part of the challenge design. The design options gave engineers different technologies to consider and potentially advance. 

“This challenge brought in new ideas from outside traditional industries and helped us identify wheel technologies that may be suitable for longer-duration surface operations,” said Lucien Junkin, robotics engineer at Johnson and co-leader of the challenge project. 

The next phase could evaluate how the wheels respond to lunar-like dust, vacuum, and extreme temperatures in Johnson’s thermal vacuum chambers. Engineers could also assess the designs over longer distances and at different sizes and loads. 

“Mobility is key to everything we want to do on the Moon,” Junkin said. “The farther we want to explore, the more we need to advance the wheel technologies that can get us there.” 

The Common Robotics Project of the Robotic Systems Technology Branch within Johnson’s Engineering Directorate conducted the Rock and Roll with NASA Challenge. NASA’s Center of Excellence for Collaborative Innovation, part of the Prizes, Challenges, and Crowdsourcing Program within the Research and Technology Mission Directorate, managed the challenge contract. Students in NASA’s Robotics Academy helped prepare hardware and support the competition, while engineers from NASA’s Glenn Research Center in Cleveland supported reviews of concepts and proposals. HeroX administered the challenge on behalf of NASA.  

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Sumer Loggins

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Our home galaxy, the Milky Way, grew to its current size in part by consuming smaller galaxies. Now, new data from NASA’s Hubble Space Telescope shows definitive evidence of a dwarf galaxy merging with the young Milky Way galaxy in the earliest phases of its evolution. This finding extends our knowledge of our galaxy’s history 1.8 billion years farther back in time than before.

The results published Monday in the journal Nature Astronomy.

The Milky Way today is a massive spiral galaxy home to hundreds of billions of stars. However, our galaxy wasn’t always so large; it has grown by forming new stars from its gas clouds as well as collecting stars, gas, and dark matter from other galaxies through mergers.

The most recent massive merger in our galaxy’s history took place with the Sagittarius dwarf galaxy, beginning over 6 billion years ago and still ongoing today. Looking back into the even more distant past, researchers learned that the Milky Way galaxy consumed another dwarf galaxy called Gaia-Sausage-Enceladus 10 billion years ago. This ancient merger greatly affected the structure of our galaxy’s disk of stars. Other, smaller mergers occurred between these two.

But our galaxy’s history doesn’t stop there. Both observations and simulations have suggested that another large merger preceded these two, though the specifics of the event have been heavily debated. Now, Hubble has uncovered definitive evidence of an earlier merger that occurred about 11.8 billion years ago, or just 2 billion years after the big bang.

“Our home is the Milky Way galaxy, but we do not know how our house was built,” said Davide Massari, lead author, Astrophysics and Space Science Observatory of Bologna in Italy. “In this paper we discover where the first significant batch of bricks came from: a dwarf galaxy that we call LKH.”

Cosmic archaeological sites

Immense astronomical surveys and precision data from spacecraft like ESA’s (European Space Agency’s) Gaia mission have been instrumental in piecing together the history of our galaxy. The farther back into our galaxy’s history that scientists attempt to look, the more difficult it becomes to tell what happened. When our galaxy was young, it was smaller and much closer in size to the galaxies it clashed with. It was also more chaotic, and it’s possible that the signs of mergers have been erased over billions of years.

It’s into this murky past that Hubble peered. Researchers used Hubble to study some of the Milky Way galaxy’s globular clusters: immense, roughly spherical collections of tens of thousands to a few million stars. Globular clusters contain some of the oldest stars in our galaxy, and they can act as cosmic archaeological sites that preserve stars from other galaxies the Milky Way galaxy has collected.

“Thanks to the high resolution and depth of Hubble imaging, we could measure the age and the metal content of these clusters with unprecedented precision,” said Chiara Zerbinati, study co-author, University of Bologna in Italy. “Coupled with measurements from Gaia, this made it possible to distinguish a population of globular clusters that are different from the others. These are the clusters that were born in LKH, and they tell us when that galaxy was devoured by ours, and how massive it was.”

The team analyzed Hubble observations of 39 globular clusters in the inner 20,000 light-years of our galaxy, where evidence of the most ancient mergers should be preserved. They expected this sample to contain globular clusters that formed within the young Milky Way galaxy as well as those collected from the Gaia-Sausage-Enceladus dwarf galaxy about 10 billion years ago.

Using Hubble’s sensitive observations to determine each cluster’s precise age and associated metallicity — the abundance of elements heavier than helium — they determined there was a third population of globular clusters in the inner regions of our galaxy. The team found that these clusters are older than the group collected in the Gaia-Sausage-Enceladus merger, but younger than those born in the Milky Way, regardless of their metal content. These  clusters, therefore, came from a separate and even earlier merger — in which the Milky Way galaxy absorbed a dwarf galaxy containing roughly 500 million times the mass of the Sun in stars, a significant fraction of our galaxy’s mass at the time. They named this dwarf galaxy Low-energy-Kraken-Heracles, or LKH, in honor of three earlier research papers that championed the idea of a merger early in our galaxy’s history.

Such a large merger so early in the Milky Way galaxy’s formation has profound implications for the evolution of our galaxy.

“Some past studies have argued that the earliest phases of our galaxy’s evolution were defined by stars born only in our galaxy,” says Massari. “Here, we have shown that stars born in external galaxies also need to be considered.”

The team plans to continue their work to unravel the history of the Milky Way galaxy by studying its globular clusters, aiming to characterize all the massive mergers that our galaxy has experienced across cosmic history.

“Hubble is observing globular clusters that have never been studied before, and this will help us characterize the merger events that are far back in time in the Milky Way galaxy’s history,” said Fernando Aguado-Agelet, co-author, University of Vigo and the University of La Laguna in Spain.

The Hubble Space Telescope has been operating for more than 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 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.

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LKH Milky Way Merger Illustration

About 12 billion years ago, a dwarf galaxy known as LKH collided with a young Milky Way and merged with it. This artist’s concept portrays that collision. NASA’s Hubble Space Telescope uncovered definitive evidence of this collision by studying globular star clusters.

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A smoke-infused pyrocumulonimbus (pyroCb) rises from the Widemouth 2 fire in Utah in these images captured by the MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Aqua satellite. The left image is natural color; the right image is false color, revealing cloud-top brightness temperatures below -40°C, a commonly used threshold for identifying pyroCbs. NASA Earth Observatory images by Michala Garrison.

Scientists have long known that volcanoes can launch large quantities of particles into the stratosphere. In the past few decades, it has become clear that wildfires do this, too, by generating towering, smoke-infused pyrocumulonimbus (pyroCb) clouds.

The largest pyroCbs are stunning weather-making features that generate massive thunderheads capable of unleashing lightning, hail, and heavy rain. A growing body of research shows that pyroCbs can also leave an outsized imprint on the upper atmosphere by channeling pulses of particles and gases into the stratosphere’s mostly dry, cloudless confines. Once there, smoke can spread widely and linger for months or years, sometimes circling the globe and likely influencing the ozone layer and Earth’s energy budget.

Understanding these enigmatic and dangerous clouds is why a team of atmospheric scientists—part of a NASA mission called INSPYRE (INjected Smoke and PYRocumulonimbus Experiment)—is spending the summer chasing them with NASA’s ER-2 aircraft, NSF/NCAR’s GV, and a suite of truck-based sensors. The team completed one of its first sampling runs of the summer on August 3, 2026, when the GV flew through a high-altitude pulse of smoke from the Widemouth 2 fire, one of Utah’s largest so far this year.

Lightning ignited the fire on July 27, 2026, but it remained relatively small until August 2, when it more than doubled in size amid intense winds and hot, dry conditions. That afternoon, soon after it had produced two pyroCb bursts, the MODIS (Moderate Resolution Imaging Spectroradiometer) on NASA’s Aqua satellite captured this image (above), showing a chimney of high-altitude cloud and smoke casting a shadow on low-altitude smoke below.

These bursts propelled clouds high enough that Aqua measured cloud-top brightness temperatures well below −40°C, a common threshold for identifying pyroCbs and a sign that the cloud tops were bubbling to the top of the troposphere and sometimes into the stratosphere. The brightness temperature measurements “reveal two discrete pulses of pyroCb action,” said Michael Fromm, a scientist at the U.S. Naval Research Laboratory. “The westernmost is the youngest pulse and stands out in the visible imagery by virtue of its shadow.”

Though relatively routine and minor, this pyroCb event followed a pre-dawn pyroCb from the same fire, imaged by the NOAA weather satellite GOES-West. “Morning pyroCbs are much more unusual,” Fromm said, because they don’t benefit from daytime heating that helps fuel convection. In this case, however, there appeared to be enough atmospheric instability and water vapor in the air to allow for pyroCb development. 

Multiple pyroCbs in a single day could have added unwanted complexity for forecasters and fire officials battling the blaze and organizing evacuations, said David Peterson, INSPYRE’s principal investigator. “Minimizing that sort of uncertainty for fire forecasters is a big part of the reason we’re out here studying this,” he added.

Remote sensing experts like Peterson and Fromm routinely study pyroCbs from afar with satellites, but it’s less common for pilots to chase and sample smoke plumes just hours after they form. In this case, the GV aircraft, on the ground in Colorado when the Widemouth 2 fire blew up, made a beeline for a high-altitude smoke plume as it drifted over New Mexico on August 3. The instruments on the plane sampled smoke at roughly 12 kilometers (8 miles) above the surface, collecting data at a height that isn’t typically incorporated into forecast models.

During that mission, a scientist on board captured this image (above) of a pyrocumulus (pyroCu) billowing up over the Widemouth 2 fire. While not as tall or energetic as pyroCbs, pyroCus are precursor clouds that share many of the same characteristics. Here, heat from the fire is fueling strong convective updrafts, forming a towering cloud with puffy overshooting tops that poke into the upper troposphere as lower-altitude smoke drifts below.

Satellites excel at identifying pyroCbs by measuring the temperature of the cloud tops that form above smoke plumes. Using this technique, researchers have established that wildfires produce about 70 pyroCbs per year, many in dense forests of Canada and Russia, though plenty also occur in grasslands and savannas in the United States and Australia. So far in 2026, Fromm and colleagues have identified at least 13 in the continental United States.

Since one of the first pyroCbs appeared in the scientific literature in the early 2000s, scientists have cataloged well over 700 events, and they now believe that wildfires may contribute up to 25 percent of the black carbon and organic aerosols in the lower stratosphere. The sheer frequency of pyroCbs means that the total mass of particles they inject over the course of a wildfire season may rival that of large volcanic eruptions.

Still, many questions about the enigmatic clouds remain unanswered. It isn’t clear what vegetation is most likely to fuel pyroCbs, why some form more lightning than others, why they form in only a small fraction of fires, and how to accurately forecast them.

“Whether it be their dangerous manifestations on the ground or their long-lasting imprint on the upper troposphere and lower stratosphere,” Fromm said, “pyroCbs continue to surprise us.”

NASA Earth Observatory images by Michala Garrison, using MODIS data from NASA EOSDIS LANCE and GIBS/Worldview. Photo by Bernadett Weinzierl/University of Vienna. Story by Adam Voiland.

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References & Resources

• CIRA CSU, via Instagram  (2026, August 3) Yesterday, the Widemouth 2 Fire in central Utah exploded. Accessed August 13, 2026.
• Denver 7, via Instagram (2026, July 28) Have you ever seen a smoke-filled cloud above a wildfire? Accessed August 13, 2026.
• The Economist (2026, August 9) NASA takes aim at fire storms. Accessed August 13, 2026.
• Fromm, M., et al. (2022) Understanding the critical elements of the pyrocumulonimbus storm sparked by high-intensity wildland fire. Communications Earth & Environment, 3, 243.
• InciWeb (2026) Widemouth 2 Fire. Accessed August 13, 2026.
• Katich, J.M. (2023) Pyrocumulonimbus affect average stratospheric aerosol composition. Science, 379(6634), 815-820.
• NASA (2026) INSPYRE. Accessed August 13, 2026.
• NASA Jet Propulsion Laboratory (2026, July 20) New NASA Earth Missions Gear Up to Start Science Flights. Accessed August 13, 2026.
• NASA Airborne Science Program (2026) Earth Science Observation Platforms. Accessed August 13, 2026.
• NASA Earth Observatory (2021, July 30) A Summer of Fire-Breathing Smoke Storms. Accessed August 13, 2026.
• NASA Earth Observatory (2020, January 10) Explosive Fire Activity in Australia. Accessed August 13, 2026.
• Peterson, D., et al. (2025) Worldwide inventory reveals the frequency and variability of pyrocumulonimbus and stratospheric smoke plumes during 2013–2023. Climate and Atmospheric Science, 8(325).
• The University of Utah (2026, August 6) Utah’s historic fire season of 2026. Accessed August 13, 2026.
• U.S. Naval Research Laboratory (2026, June 2) NRL Leads NASA Wildfire Research Mission to Better Predict Pyrocumulonimbus Storm Hazards. Accessed August 13, 2026.
• U.S. Naval Research Laboratory (2025, June 25) Fiery Storms: How Wildfires Create “Dirty Thunderstorms” and Impact Weather. Accessed August 13, 2026.
• The Weather Channel (2026, August 10) Meet the scientists who are flying into fire-breathing thunderstorms, and learn why they are doing it. Accessed August 13, 2026.
• Western Fire Chiefs (2026) Widemouth 2. Accessed August 13, 2026.
• World Meteorological Organization, Flammagenitus. Accessed August 13, 2026.

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