A lot has changed since NASA last sent astronauts to the moon — including the attitudes of those space explorers.
That's the view of Victor Glover, the NASA astronaut who served as pilot on the Artemis 2 mission around the moon's far side this past April.
"When you look back on the Apollo missions, there was a lot more competition back in the office. Everybody wanted to be the first, and then everybody wanted to be the next," Glover told Angels Broadcast Television on June 12, shortly before he threw out the first pitch before a baseball game between the Los Angeles Angels and the Tampa Bay Rays.
"I think our office learned a lot from them," he added. "There are some good things about that. It makes you work really hard, but it also can create some unnecessary conflict. And so my office really wants to support everybody — wants you to be the guy that does it, and somebody just gets picked to do it, and that's OK."
Glover and his Artemis 2 crewmates — NASA's Reid Wiseman and Christina Koch and Jeremy Hansen of the Canadian Space Agency — did indeed seem to forge a very strong bond during their training and their time in space.
For example, shortly before Artemis 2's April 1 launch, Glover, Koch and Hansen came up with a plan to name a crater on the moon after Wiseman's wife Carroll, who died of cancer in 2020.
"They said the three of them had talked, and they would like to do this," Wiseman said on April 6, the day Artemis 2 looped around the moon and got farther from Earth than any crewed mission ever had. "That was an emotional moment for me. And I just thought that was just a total treasure, that they had thought through this, and they had offered this."
Wiseman, Artemis 2's commander, said he broke down when Hansen radioed mission control with the naming request. In fact, all four astronauts were overcome with emotion at that moment.
"That was, I think, where the four of us were the most forged, the most bonded, and we came out of that really focused on that day ahead," Wiseman said.
This image taken by Buzz Aldrin of the Apollo 11 landing site is the only good picture of mission commander Neil Armstrong on the lunar surface. (Image credit: NASA)
The atmosphere was a bit different during the 1960s and early 1970s, as Glover noted; undercurrents of competition and rivalry reportedly ran through the Apollo crews.
For example, multiple people, including Apollo 17 astronaut Gene Cernan, have said that Buzz Aldrin lobbied to be the first person to set foot on the moon, an honor that eventually went to Apollo 11 crewmate Neil Armstrong. (Aldrin has disputed this version of events, saying he didn't want to be the first-ever moonwalker.)
There are other big differences between Artemis and Apollo, of course. Apollo was designed to get people to the moon before the Soviet Union could do so, a goal that was regarded as a national security imperative because it would demonstrate American technological supremacy. As a result of this need for speed, Apollo did not build anything permanent on the moon, leaving behind only flags, footprints and defunct spacecraft.
Artemis, on the other hand, aims to establish a permanent and sustainable presence on Earth's nearest neighbor. If all goes to plan, NASA will build one or more moon bases near the lunar south pole, then use the skills and knowledge gained from this endeavor to get astronauts even farther afield — to Mars.
Photographer Shane Hynan explores the tension between the central role peat bogs play in Irish life and their wider environmental impact
“You can read Ireland’s history in the boglands. They hold millennia in their layers,” says photographer Shane Hynan of his project, Beofhód (meaningBeneath in English).
The boglands, known as portachs in Irish, cover roughly 1.2m to 1.5m hectares or about 14% to 17% of the country’s total land area. The raised bogs of the Irish Midlands are made of peat that forms at a rate of 1mm a year (0.04in) in low-lying, poorly drained basins or former lakes. As the historical geographer Kevin Whelan observes in the Atlas of the Irish Rural Landscape, “the bog has been etched as deeply into the human as into the physical record in Ireland – to an extent unrivalled elsewhere.”
Eddie and Con footing turf for domestic use, Knockirr Bog, County Kildare, 2022.
NASA's plan to deorbit the International Space Station in coming years has fallen under the scrutiny of a government watchdog group and stirred up a wave of reaction by a leading ocean conservation organization.
As presently blueprinted by NASA, the International Space Station will be de-orbited via a series of actions. Firstly, in early to mid-2028, the ISS will start to be lowered through a combination of Earth's natural atmospheric drag and the execution of re-entry maneuvers by the ISS's Russian segment. Then, in mid-2029, NASA plans to launch a SpaceX-supplied, government paid for, U.S. Deorbit Vehicle (USDV) and attach that craft to the ISS, which will fire its 46 Draco thrusters and push the station down to a watery grave.
But there's one issue that has ecology experts concerned. The Ocean Foundation, a Washington, D.C.-headquartered group with a mission to improve global ocean health and the human relationship with the sea via carefully chosen strategies and projects, says the planned deorbit of the International Space Station "raises serious concerns for ocean health that the space community has not adequately grappled with," according to Mark Spalding, president of the foundation.
A troubling gap
A just-issued U.S. Government Accountability Office (GAO) report has focused on issues related to NASA's plan to bring down the International Space Station (ISS) and transition from the ISS to commercial space stations, namely NASA's concern about having a "gap" in continuous human presence in low Earth orbit.
The GAO report explains that, at the end of 2030 or early 2031, the USDV is to perform a re-entry burn. That would push the ISS through the Earth's atmosphere and into a pre-determined spot – an ocean zone called Point Nemo.
"As part of the reentry process, NASA expects portions of the ISS and deorbit vehicle to break up and fall into the remote part of the ocean to minimize the risk to populated areas," states the GAO report.
SpaceX rendering of its U.S. Deorbit Vehicle (USDV), a Dragon-derived spacecraft with 46 Draco engines designed to propel the International Space Station into a controlled reentry. (Image credit: SpaceX)
But as for using Point Nemo or any part of the ocean as a convenient dumping ground, Spalding told Space.com that "there is a troubling structural gap in international law that the ISS de-orbit throws into sharp relief."
Under the Space Liability Convention of 1972, if space debris falls on another nation's territory or damages property, Spalding said, the launching nation owes compensation - absolutely and without needing to prove fault. "But no equivalent protection exists for the ocean," he said.
"As a result, when space agencies have control over where debris falls, they aim for the high seas, and in doing so, they incur no legal obligation to pay for cleanup or environmental remediation," said Spalding.
The Ocean Foundation leader said he understood the legitimate safety rationale for targeting Point Nemo, the point on Earth farthest from any populated area. "But the ocean's remoteness from human infrastructure should not be mistaken for a lack of value or vulnerability," Spalding said. "The ocean and its creatures deserve the same protection that international law affords to national territories."
Concerning the ocean's ecosystems, Spalding asks what happens to the marine ecosystems and creatures on the seafloor where the ISS leftovers land?
"The honest answer is, we don't fully know. That is deeply troubling for a structure the size of a football field. We do know that not everything burns up on reentry. Denser components will survive and reach the seafloor," Spalding added.
Point Nemo (marked in red) in the south Pacific Ocean is farther from land than any other point on Earth. It is also home to the world's largest "Spacecraft Cemetery." (Image credit: PGC/NASA IBCAO Landsat/USGS/Google)
The problem: uncertainty
What denser, specific materials from the ISS re-entry will be, and what harm they may cause to marine life, Spalding said, "has not been adequately studied or disclosed. That uncertainty is itself the problem."
Additionally, what environmental harm may begin before the debris hits the water is worrisome. As the largest reentry in history, the cumulative atmospheric impact of down-falling ISS hardware deserves serious study, he said.
For one, Spalding flagged a newly negotiated High Seas Treaty (BBNJ Agreement) that is relevant to downing the ISS. It requires parties to conduct environmental impact assessments for activities that may affect the marine environment beyond national jurisdiction when effects are unknown or poorly understood.
"It is fair to ask whether the ISS deorbit — the largest such reentry in history, targeting the high seas — should trigger that obligation," Spalding said.
The International Space Station. (Image credit: NASA/ESA–T. Pesquet)
Position statement
As for the Ocean Foundation's position on the ISS deliberate crashing into the Pacific Ocean, the group believes that discussion points prior to the ISS downing include:
A full environmental impact assessment of the anticipated seafloor debris field and atmospheric effects;
Public disclosure of all materials that will survive reentry and reach the ocean floor;
A rigorous legal analysis of obligations under the UN Convention on the Law of the Sea (UNCLOS,) the London Protocol of 1996 that provides an international standard and framework for countries to individually and collectively protect and preserve our oceans from pollution caused by the dumping of wastes and other matter into the ocean, along with the BBNJ Agreement.
The high seas have no sovereign who can demand accountability, concluded Spalding. "We believe this gap in international law needs to be closed, and the ISS de-orbit is a vivid illustration of why."
The federal government wants to help utilities buy large components for up to 10 large nuclear reactors. It’s unclear which, if any, companies might participate.
The Vogtle nuclear power plant in Georgia is the only one with AP1000 reactors in the U.S. They generate enough electricity to power 1 million homes, but they took 15 years to build and cost $35 billion, double the initial estimates.
The federal government wants to help utilities buy large components for up to 10 large nuclear reactors. It’s unclear which, if any, companies might participate.
SpaceX's Dragon capsule leaves after dropping off some supplies and science at the ISS. (Image credit: NASA/Jessica Meir)
SpaceX's Cargo Dragon capsule shines in the sunlight over Earth as it departs from the International Space Station in a new image snapped from onboard the station.
With sunbeams gleaming downward, reflecting off of the spacecraft's hull, the Dragon can be seen backing away from the station mere moments after undocking from the port on the station's Harmony module. The undocking is so recent that you can clearly see both the docking port and the hatch of the Dragon where the two connected.
The space station has been in orbit since 1998 and continuously occupied since November, 2000. With decades of work in orbit, it can be easy to take for granted the incredible transport system that supports cutting-edge research hundreds of miles above Earth's surface.
The work done on the station is impressive, but this system is just as mind-boggling. In addition to launching and returning astronauts who perform critical maintenance and repair work on the station on top of their research duties, cargo missions keep the station stocked.
From food and clothing to medical equipment and intricate science experiments, these missions are essential for both keeping astronauts safe and healthy on station as well as continuing the progression of science in-orbit. This back-and-forth between Earth and the space station is an impressive feat, and this photo shows the system fully in-motion.
One proposal would lower the cost of the bonds that fossil fuel companies must pay the Interior Department before they start drilling or mining on public lands.
GOLDEN, Colorado – Here on Earth, centuries of accumulated engineering knowhow, hard-learned lessons, and societal evolution have shaped a robust framework of building standards that govern how we build and maintain buildings today.
But now, as humanity prepares to put in place a "sustained presence" on the moon, how do we guarantee the safety and integrity of structures built in an environment for which no such tradition exists?
At the 26th Space Resources Roundtable held June 2-5 on the campus of the Colorado School of Mines, one expert says what's needed is a lunar building code, the development of specific design criteria for the moon.
What's shaking?
Both NASA and China's space agency are planning to build habitats, landing pads, equipment shelters, and tall towers on the moon. But all that construction could be off to a shaky start, suggests Nerma Caluk, an engineer and lunar specialist for Skidmore, Owings & Merrill, an architecture and structural engineering firm in San Francisco, California.
Caluk said there's a need to leverage terrestrial building experiences.
"On Earth, structural systems rely on strong gravitational acceleration to resist seismic lateral forces through both foundation friction and overturning stability. However, on the moon, the gravitational field strength is reduced to just one-sixth of Earth's surface gravity," Caluk told Space.com.
Because seismic inertial forces are governed purely by a structure's mass rather than its weight, the lateral demand on a structure remains fully active while its gravitational restoring capacity is substantially diminished, Caluk added.
"Low-profile surface structures risk translational sliding across poorly characterized regolith interfaces, while taller vertical structures face significant overturning vulnerability, as the moon provides only a fraction of the gravitational restoring moment available in a terrestrial seismic environment," said Caluk.
Here on Earth, structural engineers routinely design typical building systems to yield, crack, and sustain permanent inelastic deformation during a design-level seismic event.
They intentionally leverage "inelastic energy dissipation" as the primary mechanism for managing seismic demand, Caluk said. But this design philosophy is fundamentally incompatible with a crewed lunar environment, she said.
Take for example a hatch distortion or pressure seal misalignment. They constitute a mission-critical failure, and any structural breach risks catastrophic depressurization, said Caluk.
An artist's rendering of a NASA Artemis moon base with development underway. (Image credit: NASA)
A group taking on the challenge of shaping guidelines on the building of lunar infrastructure is the aerospace division of the American Society of Civil Engineers.
The group's technical committee on space engineering and construction has crafted "Infrastructure Engineering, Design, Analysis, and Construction (LIEDAC) guidelines" for the moon, Caluk said, to tackle seismic issues imposed by moonquakes.
The LIEDAC guidelines, Caluk said, characterize the unique lunar hazard environment, classify operational consequences through a risk-categorization hierarchy, and establish target performance objectives "so that safe commercial development can proceed on a defensible technical basis."
Inherent uncertainties
Caluk also outlined a "Response Spectrum Analysis" supported by NASA Small Business Technology Transfer funding that looked at the inherent uncertainties of the lunar subsurface.
The output of the analysis has developed criteria emphasizing the necessity of a local geotechnical site investigation for all structures, regardless of their seismic design category.
"These investigations are critical for identifying and mitigating risks such as seismic slope stability, seismically induced total and differential settlement, and other geotechnical hazards that may be triggered or amplified by moonquake ground motions," she reported here at the School of Mines gathering.
Moreover, the framework that Caluk and her associates have pulled together, acknowledges that lunar site conditions are not yet fully understood on a global scale.
NASA envisions robotic rovers and astronauts working alongside one another to build structures on the moon. (Image credit: NASA)
Design practices
Not knowing ahead of time what lunar explorers may face is an unsure, shuddering proposition.
"Therefore, responsible design practices must account for this uncertainty through rigorous subsurface investigation whenever feasible," Caluk added. "By prioritizing localized data collection, engineers can ensure that structural foundations are robust enough to handle the unique physical properties of the lunar regolith and the specific seismic demands of the deployment site."
Caluk and her team members looked at the maximum considered moonquake, representing a more severe shaking level, to verify collapse prevention and ensure overall structural integrity under extreme lunar seismic events.
"NASA's deep institutional knowledge of human spaceflight operations and crewed mission safety," Caluk concluded, "provides the critical foundation upon which structural performance criteria for lunar infrastructure can now be formally established, with terrestrial engineering precedent offering a proven methodology for doing so even under evolving geotechnical and seismic data conditions."
NASA has announced a new commercial partnership for the next satellite headed to the Red Planet.
California-based Relativity Space will design, build and launch the spacecraft that carries NASA's Aeolus instrument suite to orbit around Mars, where the probe will be the first to provide daily measurements of the planet's global environment. Aeolus will collect data on Martian dust and cloud cover, winds and temperatures, according to a NASA release.
"Public-private partnerships like this are a force multiplier for science," NASA Administrator Jared Isaacman said in a statement on Wednesday (June 17).
The newly announced relationship, and others between NASA and private industry, is designed to allow the agency to concentrate its resources on important science discovery. "By pairing NASA’s world‑class instruments with commercial innovation and investment, we can deliver more science, more often, and reduce the time it takes to get essential data into the hands of researchers preparing for future human missions to Mars," Isaacman said.
Aeolus consists of four instruments, designed to work in tandem to create a complete picture of the Martian atmosphere and its behavior. In addition to refining scientific models for the Martian environment, NASA plans to use the data to reduce risks to future robotic and crewed missions landing on Mars' surface.
The science suite includes the Doppler Wind and Temperature Sounder (DWTS‑Ozone), in collaboration with GATS, designed to measure wind speeds and temperatures present up to 37 miles (60 kilometers) above the ground. The Thermal Limb Sounder (TLS), designed with Xiomas Technologies, will create vertical temperature profiles and provide data on atmospheric dust and cloud cover, while the Surface Radiometric Sensor Package (SuRSeP) collects compositional data on those clouds and dust, and tracks how the Martian surface absorbs, stores and releases energy, like heat. Finally, Aeolus' Wide‑Field Context Camera (WFCC) will take daily images to assess atmospheric activity across the whole of Mars.
Relativity Space's Terran 1 rocket successfully blasted off for its test flight but malfunctioned three minutes after liftoff. (Image credit: Relativity Space)
NASA is targeting 2028 for the launch of the Aeolus mission, which will be designed and built at NASA's Ames Research Center in California, where it will also be integrated on Relativity's spacecraft for testing ahead of launch. NASA has committed to support Aeolus' scientific operations for at least one Martian year (approximately 687 Earth days). However, the agency has historically extended its missions to Mars, when able.
NASA was recently forced to end operations of its MAVEN (Mars Atmosphere and Volatile Evolution) probe around Mars, after an anomaly led to a loss of communications with the satellite, but the spacecraft ran for more than a decade beyond its original one-year mission. The agency's only two active satellites orbiting the Red Planet are the Mars Reconnaissance Orbiter (MRO) and Mars Odyssey, which are both operating nearly two decades or more, respectively, beyond their initial mission timelines.
For its part, Relativity will be in charge of designing the Mars-bound spacecraft and will also be responsible for launch and for satellite operations in space. The company's pathfinder launch vehicle, the Terran 1 rocket, lifted off for the first and only time in March 2023, but it failed to reach orbit. The company then pivoted to development of the bigger, partially reusable Terran R rocket, which is expected to debut sometime later this year. Eric Schmidt, who served as Google CEO from 2001 to 2011, was appointed to lead Relativity in March 2025.
Even small asteroids lead complex lives. During its flyby of the asteroid Donaldjohanson last year, NASA’s Lucy spacecraft revealed the asteroid to be a wobbly, peanut-shaped body that has undergone a lot of activity in its relatively short history. Formed as fragments coalesced after a violent collision 155 million years ago, the asteroid was transformed by the small but inexorable force of the Sun’s radiation, all while retaining signs of the brief presence of liquid water in its distant past.
Zooming through the main asteroid belt toward one of the Jupiter Trojan asteroid groups, the Lucy spacecraft collected the first close-up images and other data at Donaldjohanson on April 20, 2025, as it passed 650 miles away from the asteroid. The data revealed that, instead of spinning simply around one axis like most other asteroids and planets, Donaldjohanson has a more complicated two-axis rotation. Scientists also saw Donaldjohanson’s peanut shape and the craters and ridges on its surface.
A timelapse video made from images taken by NASA’s Lucy spacecraft as it approached the asteroid Donaldjohanson on April 20, 2025. The L’LORRI (Lucy Long Range Reconnaissance Imager) instrument, the spacecraft’s high-resolution black-and-white imager, collected these images over two hours as the spacecraft rapidly closed in on the asteroid from an initial separation of more than 58,000 miles (93,000 km), until the spacecraft passed a mere 650 miles (1000 km) from the 5-mile- (8 km-) wide asteroid.
NASA/Goddard/SwRI/JHU-APL
Lucy’s encounter with the asteroid was planned as a dress rehearsal for the spacecraft and mission team before its primary asteroid encounters, which begin with Lucy’s flyby of the Trojan asteroid Eurybates on Aug. 12, 2027. The instruments performed as expected, and, as a bonus, scientists got a rare opportunity to study a previously unexplored asteroid up close and to compare it to two asteroids with similar compositions but different histories: Bennu, the target of NASA’s OSIRIS-REx sample-return mission, and Ryugu, the site of JAXA’s (Japan Aerospace Exploration Agency) Hayabusa2 sample-return mission.
With Earth-based telescopes, observers saw fluctuations in the light Donaldjohanson reflects, regular patterns of peaks and valleys, typical of an elongated object rotating once every 10.5 Earth days. But Lucy’s data revealed another pattern: Donaldjohanson appears to be rotating like a wobbly top. Paper authors reported that the asteroid rotates end-over-end once every 10.5 Earth days, and wobbles back and forth around its long axis once every 26.5 days.
The asteroid Donaldjohanson is shown slowly rotating in a tumbling, non-principal axis motion, with its angular momentum vector and rotation axes indicated. The surface is colored by gravity slope, which measures the angle between the local surface and the direction of gravity. Higher values (warmer colors) indicate steeper terrain relative to the local gravitational pull. Regions with limited stereo image coverage have been masked out where the shape model is less well constrained.
Kel Elkins/NASA’s Science Visualization Studio/DLR
Peanut shape
While the Earth-based observations hinted at Donaldjohanson’s elongated shape, the Lucy flyby revealed a “bilobate” structure: two lobes connected by a neck, like a peanut. These lobes are likely two fragments from an asteroid collision that gently came together afterward by their mutual gravity.
Donaldjohanson likely rotated at least 10 times faster when it formed, having slowed to its current rate in the last 20 to 60 million years, the team estimates. As it slowed, the balance between the centrifugal force pushing things apart and gravity pulling things together changed and loose rocky material slid down slopes creating the worn-down appearance of many craters, as the flyby images showed.
The paper’s authors say that the asteroid’s slowing rotation is likely caused by a subtle consequence of solar heating known as the YORP effect. Each part of the asteroid’s Sun-warmed surface radiates heat away as infrared light, and that radiation imparts a tiny recoil force to the surface. Because the asteroid’s shape isn’t symmetric, this results in a net torque, or twist, that can change the asteroid’s rotation. Thus, YORP can slow asteroid spins down or speed them up, as in the case of Bennu (once every four hours) and Ryugu (once about every seven hours), which both likely used to rotate much slower than they do today.
Fleeting water
As it passed by Donaldjohanson at 30,000 mph, Lucy recorded the signatures of iron-rich clay minerals on the surface. These clays must have formed in the distant past with the help of liquid water. However, the exposure must have been brief, Lucy scientists concluded, because iron in clays tends to be replaced with other elements, such as magnesium, as water lingers.
Indeed, scientists saw magnesium-rich clays at Bennu and Ryugu, which suggested prolonged water exposure, perhaps lasting millions of years, when they were still part of larger asteroids.
This difference in water exposure history, and other characteristics, may mean that the parent bodies of these asteroids formed at different times or in different regions of the solar system before relocating to the main belt.
Compare, contrast
Donaldjohanson is thought to be made from rocky remnants of a larger, carbon- and water-rich asteroid that collided with another object in the main asteroid belt. Bennu and Ryugu are thought to have formed in the same way and in the same region.
But Donaldjohanson is different. At 155 million years old, it is much younger than Bennu and Ryugu, which formed 1 to 2 billion years ago. Donaldjohanson also has remained in the asteroid belt since birth, while its wandering cousins migrated into orbits around the Sun that bring them close to Earth’s orbit about once a year (which made them perfect close targets for sample return missions).
During its April 20, 2025, encounter with the main-belt asteroid Donaldjohanson, NASA’s Lucy spacecraft discovered evidence for iron-rich clays on the surface using its infrared spectrometer. These clays, which are similar to those found in carbon-rich meteorites such as QUE 97990, indicate that water was briefly present in the asteroid during the distant past.
NASA/Goddard/SwRI/Dan Gallagher
“It’s helpful for scientists to compare Donaldjohanson with asteroids like Bennu and Ryugu, which are seemingly similar asteroids, because every subtle difference is another clue to our origin story,” said Simone Marchi, Lucy deputy principal investigator and lead author of the study at the Boulder, Colorado, office of the Southwest Research Institute.
“Once we start learning more about the Trojans, a completely different population of space rocks with very different histories, our understanding of solar system formation is destined to be challenged,” said Marchi.
Named after a fossilized skeleton of a human ancestor discovered in Ethiopia in 1974, NASA’s Lucy will be the first mission to explore Jupiter’s Trojan asteroids, a population of well-preserved space rocks that formed early in our solar system’s history and could help scientists understand how the planets formed and moved around before settling in their current configuration.
Lucy’s principal investigator is based out of the Boulder, Colorado, branch of Southwest Research Institute, headquartered in San Antonio. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, provides overall mission management, systems engineering, and safety and mission assurance. Lockheed Martin Space in Littleton, Colorado, built the spacecraft. Lucy is the 13th mission in NASA’s Discovery Program. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Discovery Program for the agency’s Science Mission Directorate in Washington.
For more information on NASA’s Lucy mission, visit:
Zooming through the main asteroid belt toward one of the Jupiter Trojan asteroid groups, the Lucy spacecraft collected the first close-up images and other data at Donaldjohanson on April 20, 2025, as it passed 650 miles away from the asteroid. The data revealed that, instead of spinning simply around one axis like most other asteroids and planets, Donaldjohanson has a more complicated two-axis rotation. Scientists also saw Donaldjohanson’s peanut shape and the craters and ridges on its surface.
Even small asteroids lead complex lives. During its flyby of the asteroid Donaldjohanson last year, NASA’s Lucy spacecraft revealed the asteroid to be a wobbly, peanut-shaped body that has undergone a lot of activity in its relatively short history. Formed as fragments coalesced after a violent collision 155 million years ago, the asteroid was transformed by the small but inexorable force of the Sun’s radiation, all while retaining signs of the brief presence of liquid water in its distant past.
Zooming through the main asteroid belt toward one of the Jupiter Trojan asteroid groups, the Lucy spacecraft collected the first close-up images and other data at Donaldjohanson on April 20, 2025, as it passed 650 miles away from the asteroid. The data revealed that, instead of spinning simply around one axis like most other asteroids and planets, Donaldjohanson has a more complicated two-axis rotation. Scientists also saw Donaldjohanson’s peanut shape and the craters and ridges on its surface.
A timelapse video made from images taken by NASA’s Lucy spacecraft as it approached the asteroid Donaldjohanson on April 20, 2025. The L’LORRI (Lucy Long Range Reconnaissance Imager) instrument, the spacecraft’s high-resolution black-and-white imager, collected these images over two hours as the spacecraft rapidly closed in on the asteroid from an initial separation of more than 58,000 miles (93,000 km), until the spacecraft passed a mere 650 miles (1000 km) from the 5-mile- (8 km-) wide asteroid.
NASA/Goddard/SwRI/JHU-APL
Lucy’s encounter with the asteroid was planned as a dress rehearsal for the spacecraft and mission team before its primary asteroid encounters, which begin with Lucy’s flyby of the Trojan asteroid Eurybates on Aug. 12, 2027. The instruments performed as expected, and, as a bonus, scientists got a rare opportunity to study a previously unexplored asteroid up close and to compare it to two asteroids with similar compositions but different histories: Bennu, the target of NASA’s OSIRIS-REx sample-return mission, and Ryugu, the site of JAXA’s (Japan Aerospace Exploration Agency) Hayabusa2 sample-return mission.
With Earth-based telescopes, observers saw fluctuations in the light Donaldjohanson reflects, regular patterns of peaks and valleys, typical of an elongated object rotating once every 10.5 Earth days. But Lucy’s data revealed another pattern: Donaldjohanson appears to be rotating like a wobbly top. Paper authors reported that the asteroid rotates end-over-end once every 10.5 Earth days, and wobbles back and forth around its long axis once every 26.5 days.
The asteroid Donaldjohanson is shown slowly rotating in a tumbling, non-principal axis motion, with its angular momentum vector and rotation axes indicated. The surface is colored by gravity slope, which measures the angle between the local surface and the direction of gravity. Higher values (warmer colors) indicate steeper terrain relative to the local gravitational pull. Regions with limited stereo image coverage have been masked out where the shape model is less well constrained.
Kel Elkins/NASA’s Science Visualization Studio/DLR
Peanut shape
While the Earth-based observations hinted at Donaldjohanson’s elongated shape, the Lucy flyby revealed a “bilobate” structure: two lobes connected by a neck, like a peanut. These lobes are likely two fragments from an asteroid collision that gently came together afterward by their mutual gravity.
Donaldjohanson likely rotated at least 10 times faster when it formed, having slowed to its current rate in the last 20 to 60 million years, the team estimates. As it slowed, the balance between the centrifugal force pushing things apart and gravity pulling things together changed and loose rocky material slid down slopes creating the worn-down appearance of many craters, as the flyby images showed.
The paper’s authors say that the asteroid’s slowing rotation is likely caused by a subtle consequence of solar heating known as the YORP effect. Each part of the asteroid’s Sun-warmed surface radiates heat away as infrared light, and that radiation imparts a tiny recoil force to the surface. Because the asteroid’s shape isn’t symmetric, this results in a net torque, or twist, that can change the asteroid’s rotation. Thus, YORP can slow asteroid spins down or speed them up, as in the case of Bennu (once every four hours) and Ryugu (once about every seven hours), which both likely used to rotate much slower than they do today.
Fleeting water
As it passed by Donaldjohanson at 30,000 mph, Lucy recorded the signatures of iron-rich clay minerals on the surface. These clays must have formed in the distant past with the help of liquid water. However, the exposure must have been brief, Lucy scientists concluded, because iron in clays tends to be replaced with other elements, such as magnesium, as water lingers.
Indeed, scientists saw magnesium-rich clays at Bennu and Ryugu, which suggested prolonged water exposure, perhaps lasting millions of years, when they were still part of larger asteroids.
This difference in water exposure history, and other characteristics, may mean that the parent bodies of these asteroids formed at different times or in different regions of the solar system before relocating to the main belt.
Compare, contrast
Donaldjohanson is thought to be made from rocky remnants of a larger, carbon- and water-rich asteroid that collided with another object in the main asteroid belt. Bennu and Ryugu are thought to have formed in the same way and in the same region.
But Donaldjohanson is different. At 155 million years old, it is much younger than Bennu and Ryugu, which formed 1 to 2 billion years ago. Donaldjohanson also has remained in the asteroid belt since birth, while its wandering cousins migrated into orbits around the Sun that bring them close to Earth’s orbit about once a year (which made them perfect close targets for sample return missions).
During its April 20, 2025, encounter with the main-belt asteroid Donaldjohanson, NASA’s Lucy spacecraft discovered evidence for iron-rich clays on the surface using its infrared spectrometer. These clays, which are similar to those found in carbon-rich meteorites such as QUE 97990, indicate that water was briefly present in the asteroid during the distant past.
NASA/Goddard/SwRI/Dan Gallagher
“It’s helpful for scientists to compare Donaldjohanson with asteroids like Bennu and Ryugu, which are seemingly similar asteroids, because every subtle difference is another clue to our origin story,” said Simone Marchi, Lucy deputy principal investigator and lead author of the study at the Boulder, Colorado, office of the Southwest Research Institute.
“Once we start learning more about the Trojans, a completely different population of space rocks with very different histories, our understanding of solar system formation is destined to be challenged,” said Marchi.
Named after a fossilized skeleton of a human ancestor discovered in Ethiopia in 1974, NASA’s Lucy will be the first mission to explore Jupiter’s Trojan asteroids, a population of well-preserved space rocks that formed early in our solar system’s history and could help scientists understand how the planets formed and moved around before settling in their current configuration.
Lucy’s principal investigator is based out of the Boulder, Colorado, branch of Southwest Research Institute, headquartered in San Antonio. NASA’s Goddard Space Flight Center in Greenbelt, Maryland, provides overall mission management, systems engineering, and safety and mission assurance. Lockheed Martin Space in Littleton, Colorado, built the spacecraft. Lucy is the 13th mission in NASA’s Discovery Program. NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Discovery Program for the agency’s Science Mission Directorate in Washington.
For more information on NASA’s Lucy mission, visit:
Zooming through the main asteroid belt toward one of the Jupiter Trojan asteroid groups, the Lucy spacecraft collected the first close-up images and other data at Donaldjohanson on April 20, 2025, as it passed 650 miles away from the asteroid. The data revealed that, instead of spinning simply around one axis like most other asteroids and planets, Donaldjohanson has a more complicated two-axis rotation. Scientists also saw Donaldjohanson’s peanut shape and the craters and ridges on its surface.
Top 10% generate climate and biodiversity damage bill that exceeds economies of most countries, say researchers
The environmental damage bill racked up by the highest-consuming 10% of the world’s population has reached up to $5.7tn a year – larger than the economy of every country except the US and China, a study has found.
Mega-consumers in this group are concentrated in the global north, accounting for more than half the population of the US and 40-45% of people in the EU.
It’s the third such deal the Interior Department has struck to pay firms to abandon plans for offshore turbines, spending roughly $2.5 billion to get companies to abandon their wind projects.
It’s the third such deal the Interior Department has struck to pay firms to abandon plans for offshore turbines, spending roughly $2.5 billion to get companies to abandon their wind projects.
In the relentless quest to uncover signs of life beyond Earth, scientists have turned their gaze towards the mysterious realms of ocean worlds—icy moons like Enceladus, Europa, and Titan. These celestial bodies harbor vast, hidden oceans beneath their frozen crusts, creating environments that could potentially support life. Yet, the challenge remains daunting: distinguishing genuine biological signatures from complex abiotic processes that could mimic these signals. A groundbreaking study recently published in Nature Astronomy proposes a sophisticated quantitative framework designed to rigorously evaluate these abiotic baselines on ocean worlds, shedding new light on how future life detection missions might navigate this delicate terrain.
Ocean worlds have captivated astrobiologists not merely because they contain liquid water, a fundamental criterion for habitability, but also because they offer diverse chemical environments where life as we know it might exist. However, confirming the presence of life requires more than spotting chemicals commonly associated with biology; it demands a nuanced understanding of how non-biological processes could generate similar signals, muddying the interpretative waters. The novel framework developed by Higgins, Chen, Warr, and colleagues provides an unprecedented approach to dissect this ambiguity, employing Enceladus as a primary example to demonstrate its utility.
At the heart of the study lies the challenge of interpreting isotopic measurements, particularly of methane (CH₄) and carbon dioxide (CO₂), molecules widely regarded as potential biosignatures due to their roles in Earth’s carbon cycle. The study scrutinizes the isotopic ratios of these molecules, expressed as δ¹³C values, which reflect the ratio of carbon-13 to carbon-12 isotopes. Traditionally, biological processes tend to prefer lighter isotopes, leading to distinctive fractionation patterns. However, the researchers highlight that uncertainties inherent in abiotic chemistry within Enceladus’ ocean and vent systems can produce isotopic signatures overlapping with those produced by biological activity, thereby defying straightforward interpretation.
The implication is profound: future missions that might measure δ¹³C in carbon-bearing molecules emanating from Enceladus’ plumes could misinterpret data, either falsely declaring a biosignature or overlooking subtle hints of life concealed beneath abiotic noise. The framework thus urges caution against over-reliance on isotopic biosignatures without a comprehensive assessment of the abiotic baseline. This is a pivotal insight that recalibrates how missions might prioritize scientific instruments and analytical strategies aboard orbiters or landers.
Complementing isotopic analysis, the study explores amino acid chirality as an alternative biosignature. Chirality, the “handedness” of molecules, is a hallmark of terrestrial biology, as living organisms almost exclusively synthesize left-handed amino acids. Nevertheless, the researchers caution that abiotic synthesis of amino acids on ocean worlds, influenced by factors such as radiation, mineral surfaces, and catalytic processes, could yield racemic mixtures or even chiral excesses unrelated to life. This ambiguity necessitates robust characterization of abiotic organic chemistry before interpreting chirality as a definitive biosignature in extraterrestrial contexts.
Another layer of complexity arises from the physical and geological attributes of the ocean worlds themselves. The study emphasizes that factors like internal temperature gradients, rheology (the deformation behavior of the icy shell and underlying materials), and lithology (rock types beneath the ocean) significantly influence abiotic chemical pathways. Understanding these properties with finer precision could narrow the range of isotopic and chemical signatures attributable to non-biological processes, thereby enhancing the confidence in detecting life.
Central to reducing the abiotic baseline uncertainty is the challenge of constraining the internal temperatures of ocean worlds. The framework points out that if internal temperatures can be pinpointed within a range of about 10 to 100 degrees Celsius, models of abiotic chemistry become markedly more predictive. Doing so would help delineate which molecular signals likely stem from hydrothermal activity and mineral interactions rather than biogenic outputs. This underscores the vital role of geophysical observations, such as gravity mapping, heat flux measurements, and ice shell thickness determinations, in complementing chemical analyses.
Transport timescales within the ocean and the overlying ice shell also feature as critical parameters. The timeframe over which molecules or small organic compounds travel from the ocean floor to the surface can alter their chemical and isotopic signatures dramatically. For instance, longer transport times may lead to isotopic exchanges or degradation processes that obscure the original biosignature signal. Hence, understanding ocean circulation patterns and ice shell permeability is integral to accurately interpreting any detected anomaly.
Expanding beyond Enceladus, the framework’s holistic approach is applicable to other ocean worlds such as Europa and Titan, each with their distinct environments and chemical contexts. On Europa, for example, the ocean’s interaction with a silicate seafloor and potential radiolysis-driven chemistry creates a different abiotic baseline compared to Enceladus. Titan’s complex organic-rich atmosphere and potential subsurface oceans add further layers of chemical diversity. The framework enables tailoring of life detection strategies and biosignature interpretations to these distinct habitats.
The study’s methodology can also inform future mission design, influencing instrument selection, sampling strategies, and data interpretation pipelines. By anticipating where abiotic ambiguity is most pronounced, mission planners can prioritize measurements that either better constrain abiotic baselines or provide multiple independent biosignature lines of evidence. This may include coupling isotopic data with mineralogical, geophysical, and molecular chirality information to build a more integrated and less ambiguous picture of habitability.
Furthermore, the framework embodies a precautionary principle against false positives and false negatives. Past and ongoing searches for life beyond Earth have grappled with ambiguous signals, from Viking’s methyl chloride controversy on Mars to debates over methane on the Red Planet. The ocean worlds’ complex chemistry and challenging environments elevate this problem, making a rigorous, quantitative approach like that offered by Higgins et al. indispensable in the life detection toolkit.
Importantly, this work illustrates the multidisciplinarity essential in astrobiology. Geochemistry, planetary science, biology, and physics converge to piece together the puzzle of extraterrestrial biosignatures. The framework’s integrated perspective exemplifies the collaborative spirit needed to interpret subtle clues from distant worlds and avoid the pitfalls of isolated or oversimplified analyses.
Looking ahead, technological advancements in both remote sensing and in situ exploration promise to enhance constraints on ocean world environments, thereby sharpening the framework’s applicability. For instance, sophisticated flyby missions or landers equipped with mass spectrometers, isotopic analyzers, and chiral detection capabilities may provide richer datasets. Simultaneously, laboratory simulations and terrestrial analog studies will refine models of abiotic chemistry and kinetics under relevant conditions.
The impact of this research extends beyond ocean worlds to the broader quest for life in the cosmos. The principles of robustly addressing abiotic baselines and embracing interdisciplinary data fusion can guide biosignature evaluation on exoplanets and other planetary bodies where life’s chemical fingerprints, if present, might be similarly elusive or confounded by non-biological processes.
In conclusion, the study spearheaded by Higgins and colleagues fundamentally reshapes our approach to biosignature interpretation on ocean worlds. By proposing a quantitative, comprehensive framework that weighs biosignature potential against carefully characterized abiotic backgrounds, it sets a new standard for rigor in the search for extraterrestrial life. As humanity’s exploration of the Solar System’s ocean realms advances, this framework will be pivotal in ensuring that claims of discovering life are grounded in unambiguous, scientifically defensible evidence.
Subject of Research: Evaluation of biosignature potential versus abiotic baselines on ocean worlds in the Solar System.
Article Title: A framework for evaluating biosignature potential against the abiotic baseline on ocean worlds.
Article References:
Higgins, P.M., Chen, W., Warr, O. et al. A framework for evaluating biosignature potential against the abiotic baseline on ocean worlds. Nat Astron (2026). https://doi.org/10.1038/s41550-026-02893-8
NASA will discuss an ambitious mission to boost the orbit of its Swift space telescope during a press conference today (June 17), and you can listen to it live.
In a breakthrough that could reshape the future of sustainable materials and energy production, researchers at the University of Pittsburgh’s Swanson School of Engineering have unveiled a revolutionary method of producing high-quality graphite at significantly lower temperatures than those traditionally required. The pivotal discovery emerged unexpectedly in the laboratory of Professor Götz Veser, where ethane was pumped through molten metal heated to under 1,000 degrees Celsius. Contrary to expectations, the carbon byproduct that surfaced was not the usual mundane residue but a fluffy, high-grade graphite, a material that has become a cornerstone in advanced battery technologies.
Graphite, often hailed as “black gold,” particularly in contexts involving automotive and high-tech sectors, is indispensable for lithium-ion batteries that power electric vehicles and modern electronics. Currently, the industrial synthesis of such graphite is a notoriously energy-heavy process necessitating temperatures approaching 3,000 degrees Celsius. Moreover, the global supply chain is heavily dependent on China, which accounts for some 95 percent of battery-grade graphite production. This dependency presents significant challenges in energy efficiency, sustainability, and geopolitical autonomy.
The Pittsburgh team, led by Professor Veser and former PhD candidate Aime Laurent Twizerimana, along with Assistant Professor Mohammad Masnadi and PhD student Nader Sawtarie, recognized the urgent need for an energy-efficient and domestically viable alternative. Their research harnessed an underexplored catalytic method involving molten metals, a concept that traces its roots back nearly a century but remained largely unexploited in this context. Unlike conventional solid catalysts, molten metal catalysts offer a unique physical characteristic: their extreme density causes carbon to separate and float atop the molten medium, simplifying collection and preventing reactor clogging.
The process began as an effort to develop greener pathways for ethylene production by “cracking” ethane, a major component of natural gas abundant in Western Pennsylvania. Ethane cracking conventionally involves steam reforming, a technique plagued by continuous formation of carbon deposits that necessitate frequent shutdowns for maintenance. However, the molten metal catalysis technique demonstrated a cleaner and more efficient alternative, reducing energy input while producing valuable byproducts.
As Twizerimana delved deeper into his doctoral research, he noticed a curious variation in carbon morphology when different metals were employed. Some metals yielded a fluffy, distinct carbon arrangement rather than the dense deposits typically associated with ethane cracking. This observation spurred further analysis by Sawtarie, whose expertise in two-dimensional metals and graphene characterization was instrumental. Their collaboration revealed that this fluffy substance was, in fact, high-value graphite, matching or exceeding quality standards for battery applications.
This discovery not only offers a lower-temperature route for graphite synthesis but simultaneously generates hydrogen as a co-product. Hydrogen, widely recognized as a clean energy vector, complements the sustainability credentials of this novel process by providing an additional revenue stream and reducing reliance on fossil-fuel-based hydrogen production methods.
Revolutionizing a process that typically demands prolonged batch operations at scorching temperatures—often taking up to three weeks—this new method offers a continuous, scalable approach that could dramatically reduce carbon emissions and costs. While small-scale graphite production in the United States exists, it remains economically uncompetitive compared to Chinese imports. The Pittsburgh innovation aims to close this gap by delivering domestic, scalable, and cost-effective graphite synthesis.
Supported by the University of Pittsburgh’s Big Idea Center, which provides vital mentorship and resources for entrepreneurial ventures, the research team transitioned their laboratory success into a startup named Graphonos Materials. The startup’s disruptive technology captured the imagination of investors and judges alike, securing a $20,000 Aramco Innovator Prize at the prestigious Rice Business Plan Competition—an event often dubbed the “Super Bowl” of entrepreneurial pitch contests.
Beyond financial endorsements, these achievements underscore the market’s clear appetite for sustainable, low-cost graphite and the critical role such materials play in the clean energy transition. The team is currently advancing toward developing a fully integrated bench-scale system capable of producing kilograms of graphite per day. This milestone is a crucial stepping stone toward pilot-scale demonstrations and eventual commercialization, aligning with global efforts to localize critical materials supply chains and innovate energy-efficient manufacturing.
If realized at scale, the process promises dual environmental and economic benefits by transforming Western Pennsylvania’s ethane reserves into essential raw materials that undergird electric vehicles, renewable energy storage, and advanced electronics. It embodies a strategic pivot from traditional fossil fuel processing to value-added chemical production within a circular economy framework, contributing meaningfully to energy transition narratives.
As the demand for lithium-ion batteries accelerates worldwide, fueled by electrification policies and consumer preferences, the importance of sustainable graphite synthesis cannot be overstated. The Pittsburgh innovation leverages unique catalytic chemistry and materials science to disrupt entrenched production paradigms marked by extreme energy consumption and geopolitical bottlenecks.
Ultimately, this development is emblematic of how interdisciplinary research—melding chemical engineering, materials science, and entrepreneurship—can yield tangible solutions to pressing global challenges. By capturing the potential of molten metal catalysis, the Graphonos Materials team paves the way for greener, domestic production pathways that harmonize economic competitiveness with environmental stewardship.
Subject of Research:
Advanced molten metal catalytic process for low-temperature synthesis of battery-grade graphite and hydrogen co-production.
Article Title:
University of Pittsburgh Researchers Innovate Low-Temperature Molten Metal Catalysis to Produce Sustainable Battery-Grade Graphite
News Publication Date:
April 2024
Web References:
University of Pittsburgh Swanson School of Engineering Faculty Pages
As the world continues to witness unprecedented growth in air travel, a groundbreaking study published in Communications Earth & Environment reveals alarming insights into the global repercussions of accelerating aircraft emissions on air quality and human health. This landmark research meticulously quantifies how expanding aviation activities contribute to deteriorating atmospheric conditions and exacerbate public health crises worldwide, underscoring an urgent need for global policy interventions and technological innovation.
The aviation sector, responsible for a substantial portion of anthropogenic greenhouse gas and pollutant outputs, has long been scrutinized for its environmental footprint. Yet, the intricate dynamics linking aircraft emissions to widespread air quality degradation and subsequent health implications have remained largely underexplored until now. Quadros, Nelen, Snellen, and colleagues harnessed sophisticated atmospheric modeling techniques combined with epidemiological data to elucidate these complex pathways with unprecedented precision.
Aircraft engines emit a cocktail of pollutants, including nitrogen oxides (NOx), particulate matter (PM), volatile organic compounds (VOCs), and carbon dioxide (CO2). These emissions initiate a cascade of atmospheric chemical reactions, creating secondary pollutants such as ozone and fine particulate matter, which profoundly impair air quality. The study’s simulation results reveal that aircraft emissions alone contribute significantly to elevated ground-level ozone concentrations, particularly in densely populated and heavily trafficked air corridors.
One of the study’s pivotal findings focuses on the spatial distribution of pollution burdens. Regions adjacent to major airports and common flight routes exhibit air quality dips notably beyond local vehicular and industrial contributions. The researchers found that the transboundary nature of aircraft emissions facilitates the transport of chemically reactive species across continents, linking aviation activities not only to local but also to regional and global air pollution episodes.
In terms of human health, the implications are disturbing. The researchers applied integrated exposure-response functions to estimate the morbidity and mortality attributable to aviation-induced pollution. Their assessments suggest a substantial increase in respiratory ailments, cardiovascular diseases, and premature deaths attributable to aircraft emissions. Particularly vulnerable populations, such as urban dwellers, children, elderly individuals, and those with preexisting conditions, face disproportionate risks.
Moreover, the study highlights the synergistic effects of aircraft emissions with other urban pollutants, exacerbating harmful synergistic interactions that amplify health risks. For instance, the NOx and VOCs emitted interact under sunlight to generate ozone, a potent respiratory irritant, and exacerbate asthma symptoms. The authors stress the importance of recognizing these nonlinear effects for robust public health policy formulation.
Climate feedback mechanisms linked to aviation emissions emerge as a critical concern in the report. The authors delineate how nitrogen oxides released at high altitudes not only affect surface-level ozone but also perturb the radiative balance of the atmosphere. This creates complex feedback loops that potentially accelerate climate warming, indicating that the environmental cost of aviation extends beyond conventional pollutants to include broader climatic impacts.
Technology advances and mitigation strategies receive thorough evaluation in the study. The authors discuss current emission reduction technologies such as lean-burn engines, sustainable aviation fuels (SAFs), and operational measures like optimized flight paths and altitude adjustments. Despite their promise, the research cautions that without comprehensive adoption and scaling, these technologies alone may fall short of offsetting the forecasted growth in emissions.
The aviation sector is projected to expand considerably over the coming decades, driven by economic growth and increasing globalization. The study’s projections indicate that without stringent regulatory frameworks and aggressive emission reduction commitments, the global burden of aviation-induced air pollution and related health impacts will escalate dramatically, particularly in emerging economies with rapidly growing air traffic.
Policy recommendations form a cornerstone of the researchers’ conclusions. They advocate for coordinated international efforts to tighten emission standards, mandate SAF usage, and invest in next-generation propulsion technologies such as electric and hydrogen-powered aircraft. Furthermore, integrating aviation sector goals into broader air quality management and climate policies is deemed essential to maximize health and environmental benefits.
In addition to technological and regulatory measures, the report emphasizes the role of real-time monitoring networks and data-sharing frameworks. Enhanced surveillance of aircraft emissions and their atmospheric transformations can enable dynamic policy responses, better inform public health advisories, and foster transparency and accountability among stakeholders ranging from airlines to regulators.
The health economics dimension discussed in the study reveals enormous societal costs tied to aviation-related air pollution. Hospitalizations, lost productivity, and long-term healthcare expenditures attributed to pollution-induced diseases impose substantial financial burdens on governments and communities alike, reinforcing the public health imperative for aggressive mitigation.
Further research priorities identified in the report call for improved characterization of ultrafine particles emitted by aircraft engines, nuanced understanding of population exposure patterns near airports, and exploration of co-benefits arising from simultaneous air quality and climate interventions. Interdisciplinary collaboration combining atmospheric science, epidemiology, engineering, and policy studies is championed as the pathway to innovative solutions.
In light of this new research, the aviation industry stands at a crossroads. Balancing the undeniable economic and social advantages of air travel with its adverse environmental and health externalities necessitates transformative thinking and collaborative global action. The study’s revelations provide an indispensable scientific foundation for stakeholders to forge a sustainable aviation future.
This comprehensive investigation serves as a clarion call for urgent recognition of the aviation sector’s hidden consequences, urging policymakers, industry players, and the public to engage in proactive, science-informed strategies that safeguard air quality and human health on a planetary scale.
Subject of Research:
The study focuses on evaluating the global impact of increasing aircraft emissions on air quality and related human health outcomes, analyzing both direct and indirect effects through sophisticated atmospheric and epidemiological modeling.
Article Title:
Global air quality and human health impacts of growing aircraft emissions
Article References:
Quadros, F.D.A., Nelen, R., Snellen, M. et al. Global air quality and human health impacts of growing aircraft emissions. Commun Earth Environ (2026). https://doi.org/10.1038/s43247-026-03732-4
Image Credits: AI Generated
DOI: 10.1038/s43247-026-03732-4
Keywords:
Aircraft emissions, air quality, human health, nitrogen oxides, particulate matter, ozone formation, aviation pollution, atmospheric modeling, public health impact, sustainable aviation fuels
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