Igniting Roman’s Journey

A SpaceX Falcon Heavy rocket launches with NASA’S Nancy Grace Roman Space Telescope onboard from Launch Complex 39A on Aug. 30, 2026, at Kennedy Space Center in Florida.
NASA/Joel Kowsky

Now on a three-month, million-mile journey to its final orbit, NASA’s Nancy Grace Roman Space Telescope will soon reveal the universe’s darkest secrets. The mission launched at 7:26 a.m. EDT on Aug. 30 aboard a SpaceX Falcon Heavy rocket from Launch Complex 39A at the agency’s Kennedy Space Center in Florida.

Roman pairs a large field of view with crisp infrared vision to explore vast swaths of the sky and probe deeply into cosmic history. This flagship mission will help astronomers explore dark matter, dark energy, and worlds outside of our solar system, known as exoplanets.

Roman is the fourth primary mission NASA has launched on a Falcon Heavy rocket. Earlier this year, the agency’s Launch Services Program worked with SpaceX to accelerate the launch date to accommodate the space telescope’s early completion.

Source: www.nasa.gov

Astronauts Anil Menon and Sophie Adenot on Spacewalk

From left, Expedition 75 flight engineers Anil Menon of NASA (partially obscured and wearing the spacesuit with a red stripe on the legs) and Sophie Adenot of ESA (European Space Agency) work outside the International Space Station.
NASA

From left, Expedition 75 flight engineers Anil Menon of NASA (partially obscured and wearing the spacesuit with a red stripe on the legs) and Sophie Adenot of ESA (European Space Agency) work together during a six‑hour and 23‑minute spacewalk outside the International Space Station on Aug. 18, 2026. The pair will finish installing a high-speed communications antenna on Aug. 25, 2026.

Watch the spacewalk live.

Image credit: NASA

Source: www.nasa.gov

NASA Sets Spacewalk for Station Maintenance, Live Coverage Planned

Expedition 74 flight engineers Sophie Adenot of ESA (European Space Agency) and Jessica Meir of NASA work together inside the International Space Station’s Quest airlock. Adenot is wearing a spacesuit in a powered and pressurized configuration to test its mobility, comfort, and optimal fit. Meir also assisted Adenot in conducting suit leak and pressure checks while verifying the suit’s communications hardware and life‑support systems.
NASA astronaut Jessica Meir and ESA (European Space Agency) astronaut Sophie Adenot work together inside the International Space Station’s Quest airlock during spacesuit fit and leak checks.
Credit: NASA

NASA will provide coverage as two astronauts step outside the International Space Station on Tuesday, Sept. 1, to replace a spacecraft navigational aid and complete several maintenance tasks in support of space station operations.

Watch live coverage beginning at 7 a.m. EDT. The spacewalk is expected to start at approximately 8:30 a.m. and last about six and a half hours. NASA’s spacewalk coverage will stream through a variety of platforms. Learn where to watch online:

https://nasa.gov/live

During U.S. spacewalk 99, NASA astronaut Jessica Meir and ESA (European Space Agency) astronaut Sophie Adenot will replace a retroreflector on the forward port of the space station’s Harmony module to support spacecraft navigation during rendezvous and docking operations. After installing the reflector, the crew will work to install jumper cables for the data-relay systems, prepare the Alpha Magnetic Spectrometer’s radiator for future maintenance, and replace a high-definition camera on the station’s truss.

Adenot will serve as spacewalk crew member 1 and will wear a suit with red stripes. Meir will serve as crew member 2 and will wear an unmarked suit.

This will be Meir’s seventh spacewalk and Adenot’s third. Meir will move into third all-time for total spacewalks among women at NASA, trailing Peggy Whitson (10) and Suni Williams (9). The excursion also marks the 284th spacewalk supporting space station assembly, maintenance, and upgrades.

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

https://www.nasa.gov/station

-end-

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

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

Details

Last Updated

Aug 26, 2026

Editor
Jennifer M. Dooren

Source: www.nasa.gov

NASA Astronaut Jonny Kim Departs Agency to Continue Military Service

NASA astronaut Jonny Kim poses for a portrait at NASA’s Johnson Space Center in Houston, Texas.
NASA astronaut Jonny Kim poses for a portrait at NASA’s Johnson Space Center in Houston.
Credit: NASA/Josh Valcarcel

After nearly a decade of service to NASA, including an eight-month science expedition aboard the International Space Station, astronaut Jonny Kim’s last day at the agency is Thursday. He will continue serving as lieutenant commander in the U.S. Navy.

Kim launched to the space station in April 2025 aboard the Soyuz MS‑27 spacecraft to conduct scientific research as a flight engineer during Expeditions 72/73. During the mission, he orbited Earth 3,920 times, traveled nearly 104 million miles, and contributed to a broad range of scientific investigations spanning technology development, Earth science, biology, and human research critical for future exploration.

“Jonny Kim represents the very best of NASA, a person who continually pushed the boundaries of exploration while inspiring countless others,” said NASA Administrator Jared Isaacman. “His contributions aboard the International Space Station advanced critical science that will shape NASA’s future missions for decades to come. We are grateful for his dedication to our nation and to the pursuit of knowledge, and we wish him success as he continues his service in the U.S. Navy.”

Serving as the U.S. Operating Segment lead for the second half of Expedition 73, Kim oversaw operations across the station’s international modules. During the expedition, the station achieved a historic milestone when every available docking port was occupied for the first time in 25 years. He also commanded the Canadarm2 robotic arm during the first capture of Northrop Grumman’s new Cygnus XL spacecraft, securing 11,000 pounds of supplies for the station. Kim and his Roscosmos crewmates landed safely in Kazakhstan in December 2025.

“Jonny has been an integral part of the agency, and his immeasurable impact will be felt for generations to come,” said Vanessa Wyche, director of NASA’s Johnson Space Center in Houston. “From advancing groundbreaking science to inspiring the next generation, Jonny has been an incredible source of inspiration to our nation. His exceptional talent, determination, and grit will leave a lasting legacy at NASA.”

Kim was selected as a NASA astronaut in 2017 and completed two years of astronaut candidate training, which included instruction in space station systems, Russian language, robotics, T‑38 flight operations, geology, survival training, and spacewalk preparation.

He later supported station operations as a capsule communicator, or capcom, in NASA’s Mission Control Center at Johnson. Kim also contributed to Artemis program development through his work in the astronaut exploration branch, leading the astronaut crew operations branch, and serving as increment lead for Expedition 65. His experiences as a Navy SEAL, physician, and naval aviator provided unique perspectives in mission operations and crew support.

“Jonny approached every assignment with humility, precision, and steadfast commitment to the mission,” said Scott Tingle, chief of the Astronaut Office at NASA Johnson. “His combination of medical training, operational experience, and engineering insight strengthened our team and contributed to advancements in exploration and space station operations.”

Born in Los Angeles, Kim enlisted in the U.S. Navy after graduating high school in 2002. He trained as a hospital corpsman and completed Basic Underwater Demolition/SEAL training before joining SEAL Team Three. Over the course of more than 100 combat operations, he served as a medic, sniper, navigator, and point man, earning the Silver Star, Bronze Star with Combat “V,” and numerous additional commendations.

He earned a bachelor’s degree in mathematics from the University of San Diego and a doctor of medicine from Harvard Medical School. He completed his internship at Massachusetts General Hospital and Brigham and Women’s Hospital in Boston. Kim became a dual-designated naval aviator and flight surgeon, completing flight training at Naval Air Stations Corpus Christi in Texas and Whiting Field in Florida, and aerospace medical training at the Naval Aerospace Medical Institute at Naval Air Station Pensacola.

Kim is returning to active duty to finish out the remainder of his military career within naval aviation training.

“Contributing to space exploration and serving NASA has been the honor of a lifetime,” said Kim. “Throughout my career, I’ve learned that beyond the missions, the training, and the hardware, success always comes down to the people. They are our greatest asset, and leading with love and empathy is how we achieve the impossible. I look forward to carrying my commitment to service, my enduring love for space and technology, and the hard-earned lessons of this past decade into my next chapter to make a meaningful impact on humanity’s future.”

To learn more about NASA’s astronauts and human space exploration, visit:

https://www.nasa.gov/astronauts

-end-

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

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

Details

Last Updated

Aug 27, 2026

Editor
Jessica Taveau

Source: www.nasa.gov

Starstruck: NASA Research Shows How Sun’s Ancient History Shaped Earth

6 Min Read

Starstruck: NASA Research Shows How Sun’s Ancient History Shaped Earth

At the center of our solar system, the Sun influences every planet that orbits it. In two recent NASA-funded studies, scientists uncovered how ancient events in the Sun’s history may have helped create Earth’s unique climate and driven previously unexplained climatic shifts.  

In new research, scientists at NASA’s SHIELD (Solar Wind with Hydrogen Ion charge Exchange and Large-Scale Dynamics) center — one of NASA’s DRIVE (Diversify, Realize, Integrate, Venture, Educate) Science Centers — trace the trajectory of the heliosphere, the massive bubble created by our Sun that envelops our solar system, as it moved through our galaxy and influenced Earth’s climate along the way. In another paper, a NASA scientist and coauthors investigate how the younger, dimmer Sun managed to heat Earth by seeding the production of potent greenhouse gases.

A Sun on the move 

Over the last tens of millions of years, Earth’s climate has undergone significant shifts, including notable ice ages in which the global average temperature temporarily dropped by several degrees. During these periods, more frequent climate swings led Earth to warm and cool. To explain these periods of warming and cooling, scientists looked to factors internal to Earth, including orbital changes, greenhouse gases, and ice. But new research suggests changes to the Sun’s environment may be key to understanding Earth’s temperature swings. 

Just as our planet is encased by an atmosphere, so our entire solar system is encased inside a kind of “atmosphere” created by the Sun. This protective bubble, known as the heliosphere, is formed by a continuous solar wind of charged particles streaming out from the Sun in all directions. 

This conceptual animation begins with a view of the Milky Way Galaxy. As we zoom in, we travel to the Local Interstellar Cloud, and then to the heliosphere, the protective bubble that surrounds our solar system. The heliosphere is formed by a continuous stream of charged particles from the Sun, called the solar wind.
NASA’s Goddard Space Flight Center Conceptual Image Lab

Our heliosphere orbits around the center of our galaxy, the Milky Way. Throughout the Sun’s 4.6-billion-year existence, our heliosphere has traversed various regions within our galaxy. In a paper published on Aug. 21 in Annual Review of Astronomy and Astrophysics, researchers at NASA’s SHIELD used computer modeling to reverse-engineer the path of the heliosphere through our galaxy, revealing that the environments it passed through may have triggered changes on Earth.   

Merav Opher, SHIELD’s principal investigator at Boston University, and her team ran simulations that showed the Sun has encountered frigid expanses of gas and dust at least three different times in the past few million years. In these instances, massive interstellar “cold clouds” pushed against the heliosphere to such an extent that it shrank to smaller than Earth’s orbit, stranding our planet outside the Sun’s protective shield. 

These exposures — approximately 2 to 3 million years, 6 to 7 million years, and 13 to 14 million years ago — would have exposed Earth’s atmosphere to totally different surroundings. The simulation results match geologic evidence: Elements prevalent in interstellar dust appear in deep-sea sediment core samples, Antarctic snow, and lunar samples during these timelines. 

This animated illustration shows Earth and the Sun protected by the heliosphere, the massive bubble created by our Sun. As our solar system traverses through the galaxy, encounters with massive interstellar “cold clouds” pushed against the heliosphere and caused the heliosphere to shrink past Earth, exposing the planet to cosmic radiation and elements from interstellar space.
NASA’s SHIELD DRIVE Science Center/Merav Opher/Harvard Radcliffe Institute

These heliosphere collapse events may also explain ancient climatic patterns on Earth. In the simulations, when Earth’s atmosphere was exposed to a cold, dense galactic hydrogen cloud, it increased water vapor content and shifted upper-atmospheric dynamics, ultimately altering the conditions at the surface. In summary, our heliosphere’s trips through colder regions in our galaxy may be a key factor in driving some of Earth’s ancient changes in climate, including possible ice ages.  

Next frontier in studying heliophysics 

The SHIELD center is one of several that NASA funds to unlock the next generation of heliospheric research. As a DRIVE Science Center, SHIELD builds a team of researchers with differing expertise, approaches, and opinions to develop a model, or “digital twin,” of the heliosphere that helps reveal how the heliosphere interacts with its surroundings, including dense interstellar clouds. Understanding our unique, habitable solar system will help unravel the mysteries of life’s evolution on Earth and potentially uncover other habitable star systems. 

Young Sun 

In another paper, Vladimir Airapetian, a scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, focuses on a long-standing mystery of how the ancient Sun warmed early Earth enough to sustain life. Three billion years ago, the young Sun was 70% as bright as it is today. Under these dimmer conditions, Earth should have been frozen solid. Yet geological evidence shows stable liquid water already existed long before that. This puzzle — a balmy Earth under a cooler, dimmer Sun — is known as the Faint Young Sun paradox.  

One clue to resolving the paradox comes from young Sun-like stars elsewhere in the galaxy. These “toddler” stars are prone to throwing fits. Specifically, data from NASA’s retired Kepler space telescope shows that young Sun-like stars regularly erupt with massive superflares, flinging high-energy particles in all directions on a daily basis. If our young Sun was like these other stars, Airapetian proposes, the barrage of high-energy solar particles could have triggered chemical reactions that were key to warming early Earth. 

Airapetian’s team simulated early Earth’s atmosphere in a sealed chamber, mixing molecular nitrogen, ammonia, carbon dioxide, and carbon monoxide. They then fired protons into the mixture, simulating the onslaught of particles from superflares. This proton bombardment triggered several changes including the production of nitrous oxide, a greenhouse gas 300 times more potent than carbon dioxide. The research was published in Astrophysical Journal Letters.

This nitrous oxide could help Earth hold onto heat. But not all the nitrous oxide would last. The young Sun’s intense ultraviolet radiation would break some of it down, splitting the molecule back into nitrogen and oxygen. But even if only 10% of the nitrous observed in the experiment survived, Airapetian’s team’s computer simulations confirmed, it would still warm Earth’s equatorial regions to about 41 degrees Fahrenheit (5 degrees Celsius), above water’s freezing point. This smaller amount of nitrous could even accelerate prebiotic synthesis: just-above-freezing temperatures have been found to be more efficient for building complex chains of amino acids than warmer temperatures. 

Unearthing secrets of our star-planet system 

Together, these two studies show that the Sun can lead to surprising implications for Earth. While our planet stands alone in many ways, it was formed and has always existed as part of a star-planet system. Understanding that unique relationship promises new insights about both Earth and the star that sustains it.  

By Desiree Apodaca and Miles Hatfield 
NASA’s Goddard Space Flight Center, Greenbelt, Md. 

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Michigan’s Les Cheneaux Islands

A portion of the Upper Peninsula of Michigan runs across the top of the image. It is mostly green, with some roads and two bright rock quarries visible. Numerous islands near the shore have elongated shapes and are oriented at a diagonal.
The Les Cheneaux Islands are a group of 36 glacially shaped islands near the Upper Peninsula of Michigan, seen in this image acquired with the OLI (Operational Land Imager) on Landsat 9 on July 23, 2026.
NASA Earth Observatory/Lauren Dauphin

With one glance at a particular 12-mile stretch of Lake Huron’s shoreline, it’s clear there’s a pattern. Small islands outlined by tan beaches and bright, shallow water align in a remarkably parallel orientation. The claw-mark-like appearance of this Great Lakes locale is evident in this image, acquired with the OLI (Operational Land Imager) on the NASA-USGS Landsat 9 satellite in July 2026.

The Les Cheneaux Islands are a group of 36 islands near the shore of Michigan’s Upper Peninsula, about 20 miles (32 kilometers) northeast of the Straits of Mackinac. The archipelago contains coastal marshes, rock and sand beaches, peat bogs, and forests full of pine and cedar. Parts of several islands are set aside as nature preserves, including a substantial portion of Marquette Island, which is only accessible by boat or over ice. The islands are interspersed with sheltered waters that inspired their name; the French “Les Cheneaux” roughly translates to “the channels.”

The Les Cheneaux Islands, like many landforms in the Great Lakes region, look the way they do because of glaciers that carved the landscape during the Wisconsin Ice Age before retreating around 10,000 years ago. Their elongated shapes indicate many of them are drumlins: mounds of glacial debris that run parallel to the direction of the ice’s movement. 

The glacial topography has helped give rise to a distinct local maritime culture. In contrast with the Great Lakes’ vast open expanses, the waters around the Les Cheneaux Islands are relatively protected from the infamous storms that can otherwise roil the upper Midwest lakes. This creates opportunities for paddling, as well as fishing in quiet alcoves for species such as smallmouth bass, northern pike, yellow perch, and lake trout. The town of Cedarville boasts an annual antique wooden boat show, a boat-building school, and museums highlighting how people, from the area’s earliest inhabitants to today’s residents, have used the islands and waterways.

On land, the much older geology of the area is revealed in a couple of brightly colored quarries. The bedrock here is dolomite, a modified form of limestone. It was deposited in the Silurian period more than 400 million years ago in a shallow, tropical sea before the movement of tectonic plates brought it up north. Michigan is home to several large dolomite and limestone mines, and Port Dolomite, east of Cedarville, ships millions of tons of the material every year.

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

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A Changing World for Emperor Penguins



1989
2025

In a satellite image captured in 1989, faint brown guano stains are visible on a background of white fast ice near a cluster of icebergs. The stains are near the edge of an ice shelf to the south.
NASA Earth Observatory/Michala Garrison

In a similar image captured in 2025, brown guano stains are still visible along the ice shelf, though the locations of icebergs.
NASA Earth Observatory/Michala Garrison

In a satellite image captured in 1989, faint brown guano stains are visible on a background of white fast ice near a cluster of icebergs. The stains are near the edge of an ice shelf to the south.
NASA Earth Observatory/Michala Garrison

In a similar image captured in 2025, brown guano stains are still visible along the ice shelf, though the locations of icebergs.
NASA Earth Observatory/Michala Garrison


1989

2025


Landsat has observed evidence of emperor penguins living on Smyley Island in Antarctica as early as 1989. The TM (Thematic Mapper) on Landsat 4 captured this false-color image (left) of guano stains on fast ice on December 24, 1989. The OLI (Operational Land Imager) on Landsat 8 captured a similar scene on December 10, 2025 (right). The images combine observations of infrared, red, and green light to make it easier to distinguish the guano stains. NASA Earth Observatory images by Michala Garrison.

With their charming waddles, heat-conserving huddles, and tuxedo-like plumage, emperor penguins are among the world’s most recognizable animals. Recent satellite surveys estimate that hundreds of thousands of the flightless birds live in 66 colonies spread around Antarctica’s inaccessible, frozen coastlines. But those numbers could fall in the coming decades because emperor penguins rely on landfast (or fast) ice—a type of sea ice attached to the shoreline—to breed, raise chicks, and molt.

While Antarctic sea ice remained relatively stable between the late 1970s and 2015, it has been declining since 2016, and climate projections suggest that trend will continue. How landfast ice is faring remains poorly understood and is an active area of study. However, one study suggests that it has declined in West Antarctica and the Weddell Sea in recent decades even as it has trended upward in the Bellingshausen Sea and East Antarctica.  

Meanwhile, some models project that emperor penguins could disappear by 2100 due to their habitats becoming inhospitable. The U.S. Fish & Wildlife Service listed emperor penguins as threatened in 2022, and the International Union for Conservation of Nature classified them as endangered in 2026.

After Antarctic sea ice cover hit a record low in 2022, British Antarctic Survey researchers reported “catastrophic” breeding failures among Bellingshausen Sea colonies. However, new research, based on decades of observations from NASA-USGS Landsat satellites, offers some hope, underscoring that many colonies have persisted for decades and that emperor penguins may be more flexible about where they breed than previously thought.

Except for a few well-studied colonies, scientists have known little about how long many emperor penguin colonies have existed, how their populations have changed, or how they have responded to past disruptions in landfast sea ice.

Three adult penguins with black-and-white plumage are surrounded by several younger penguins with fuzzy gray plumage.
Adult and juvenile emperor penguins congregate on sea ice in Antarctica.
Michael Van Woert, NOAA NESDIS, ORA

“There’s little baseline information for what’s ‘normal’ for most of these colonies,” said Michelle LaRue, a wildlife ecologist at the University of Canterbury. That’s made projecting future population levels a challenge.

Two new studies published in 2026 used decades of Landsat observations to start filling gaps in understanding. Landsat cannot resolve individual penguins, but researchers identify colonies from the guano stains that accumulate where thousands of birds congregate on the ice.

Using this technique, researchers at the University of Freiburg found that 18 colonies predate their initial identification by an average of 17 years. Because Landsat has imaged Antarctica continuously since the early 1980s, it provides one of the few systematic long-term records of remote penguin colonies.

Among the oldest colonies studied was the roughly 6,000-bird Smyley Island colony in the Bellingshausen Sea, which dates to at least 1989, two decades earlier than previously known. Other colonies that predated their earliest known presence by 20 or more years included those at Barrier Bay, Brownson, Luitpold Coast, Ragnhild, Smith, and Verdi Inlet.

Scientists have watched the Smyley Island colony closely in recent years because it is among the colonies that may have suffered a total breeding failure in 2022. Satellite images captured that year show the colony splitting up, with some penguins moving onto a large iceberg grounded near the coast.

Despite persistently low sea-ice conditions since then, the colony has continued to appear in satellite imagery, generally establishing itself near icebergs along the edge of the ice shelf. The image above on the right shows the colony in December 2025, the most recent month Landsat has observed the colony.

“We’re seeing a degree of resilience in the Smyley Island colony,” LaRue said. “They seem to be doing okay now, and we will continue to monitor them to learn more about their behaviors.” The colony’s persistence underscores that one bad breeding year—even a total failure—doesn’t mean the end of a colony. Blizzards and predators can lead to bad years with very low chick survival rates as well, she added. “It’s when we start to see frequent breeding failures year after year that the birds won’t be able to keep up, and it starts to be a problem for a colony.”

An image (left) shows a long trail of guano extending from rift ice northward to a larger guano stain on a nearby ice shelf in 2018. In 2023, brown guano stains are visible on fast ice much closer to open water, while there is no sign of the penguin colony on the ice shelf (right).
Landsat 8 captured an image of the SANAE colony with a guano trail leading from rift ice to the ice shelf on January 23, 2018 (left). On January 4, 2023, the birds had returned to their original fast ice area (right). The images combine observations of infrared, red, and green light to make it easier to distinguish the guano stains.
NASA Earth Observatory/Michala Garrison

A second study, led by Grant Macdonald, a remote sensing scientist at Durham University, found further evidence of behavioral flexibility. Macdonald and colleagues analyzed nearly 40 years of observations from Landsat, the ASTER (Advanced Spaceborne Thermal Emission and Reflection Radiometer) on NASA’s Terra satellite, and other sources for three colonies disrupted by iceberg calving or early sea ice breakup. They found that penguins of the Mertz and SANAE colonies responded by temporarily shifting to nearby icebergs, embayments, or ice shelves before returning to their former breeding sites.

Landsat first imaged the SANAE colony in 1984 on fast ice in a sheltered bay in the Queen Maud Land region in East Antarctica. After a major calving event in 2011 exposed the fast ice to more punishing winds, the colony relocated to rift ice in an embayment 11 kilometers (7 miles) to the south. The move proved temporary. Part of the group moved to another nearby site, and part of it returned to the original breeding location in 2016.

Yet in the 2016–2017 breeding season, the returnees did something unexpected. Despite the presence of stable fast ice, they trekked onto the ice shelf and huddled and bred there. In the Landsat image above, a winding guano-stained trail traces the penguins’ route onto the ice shelf. By 2022, after roughly a decade of wandering and splitting between sites, the entire colony had returned to its original breeding ground on the fast ice, where it has bred each year since.

At the third colony the researchers studied, the Astrid colony on the Vigridisen Ice Shelf, the birds kept returning to their original breeding location even after a major calving event in 2006. That’s likely because some fast ice remained and nearby icebergs provided some shelter. The guano stains indicate that the colony did, however, sometimes spend time on a nearby ice shelf toward the end of the breeding season both before and after the calving event.

Indeed, moving and sometimes breeding on alternative surfaces such as ice shelves, icebergs, or rift ice may be “more common and feasible than previously thought,” Macdonald said, perhaps because some sites offer better shelter from wind. This willingness to move may represent a “useful adaptation” as ocean temperatures warm and sea ice declines, he added, though he cautioned that behavioral flexibility alone won’t necessarily offset the long-term effects of continued sea-ice loss.

“We have so much more to learn about emperor penguins,” added LaRue. “These colonies are so remote and difficult to access that satellites—especially government satellites with easily accessible data—are going to be absolutely invaluable to understanding what the future will bring for them.”

NASA Earth Observatory images by Michala Garrison, using Landsat data from the U.S. Geological Survey. Photo by Michael Van Woert (NOAA NESDIS, ORA). Story by Adam Voiland.

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The Forested Floodplains of Congaree National Park

A brown, meandering river cuts through a band of dark green forest in Congaree National Park. Labels point out an oxbow lake and meander in the river. Former river channels called paleochannels appear lighter green than other forested areas.
The OLI on Landsat 9 captured this image of the Congaree River winding through floodplain forests in Congaree National Park on August 18, 2025.
NASA Earth Observatory/Michala Garrison

Among the 63 U.S. national parks, few are as defined by a single river’s floodplain as Congaree National Park in South Carolina. While the features are also prominent in other parks, a full 80 percent of Congaree National Park lies within the Congaree River floodplain.

It’s a place home to one of the largest intact tracts of old-growth bottomland hardwood forests in the United States. In this image captured by the OLI (Operational Land Imager) on Landsat 9, the river winds through the forested plain, along with curving bands of green that trace old channels, ridges, and swales left behind as the river gradually migrated across it. Slight differences in elevation in these paleochannels and other landforms affect how frequently they flood, producing distinct ecosystems that appear in contrasting shades of green.

The river flows through flat, soft terrain, which encourages the formation of bends and meanders. Water typically flows faster on the outside of bends, leading to more rapid erosion as the channel carves into the outer riverbank. It moves more slowly on the inside of bends, resulting in the deposition of sediment and the growth of sandy features called point bars. Over time, this process can cut off a bend from the main river channel, forming U-shaped oxbow lakes.

The National Park Service lists Weston Lake, 1.2 miles (1.9 kilometers) from the visitor center, as one of the park’s most permanent oxbow lakes, noting that it is relatively deep and lacks the shallow clay and silt layer found in most of the park’s other oxbow lakes, such as Devil’s Elbow. On the right side of the image is Bates Old River, a roughly 4-mile-long abandoned channel of the Congaree River and one of the longest oxbow lakes in South Carolina. Over time, abandoned channels and oxbow lakes can fill with sediment and become shallow wetlands. Some of these low-lying, water-filled features are known as sloughs, where flood-tolerant cypress-tupelo forests tend to grow.

While loggers targeted forests along the Congaree in the 1880s, challenges such as frequent flooding, interminably muddy roads, and mosquito-plagued conditions meant that most of the floodplain forests escaped the widespread logging that transformed other parts of the Southeast. By the 1950s, conservationists had begun to recognize how rare old-growth forests of this type had become in the region. Congress designated the area a national monument in 1976, and it became a national park in 2003.

As the river snakes its way through the park’s mostly flat terrain, it overflows its banks several times per year, usually in the winter and early spring but also in the summer and fall after hurricanes and major rainstorms. These floods distribute broad layers of nutrient-rich silt throughout the floodplain, nourishing the forests and contributing to the high concentration of unusually large trees in the park.

Over the decades, Congaree National Park has harbored a remarkable array of giant “champion” trees that have held national and state size records for their species. Though individual trees have gained and lost champion status as they have been damaged, have died, or been surpassed by newly measured trees elsewhere, Congaree trees such as the possumhaw (Ilex decidua), water hickory (Carya aquatica), loblolly pine (Pinus taeda), laurel oak (Quercus laurifolia), swamp tupelo (Nyssa biflora), and sweetgum (Liquidambar styraciflua) have held records at times.

During this National Park Week, celebrate by exploring Earth Observatory’s U.S. National Parks from Space collection. You can also check out the offerings of Earth to Sky, a collaborative program that connects NASA science with park service rangers across the nation.   

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

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A Trio of Tropical Cyclones in the Pacific

In a full-disk satellite view of Earth, three tropical cyclones—named Lowell, Karina, and Marie—swirl above the blue waters of the Pacific Ocean and to the west of Central America.

When hurricane forecasters released their seasonal outlooks in spring 2026, the El Niño brewing in the Pacific contributed to predictions of below-normal activity in the Atlantic basin but above-normal activity in the northeastern and central Pacific basins. In early September, near the climatological peak of hurricane season, those spring outlooks were on target, with the eastern Pacific buzzing with activity and the Atlantic notably quiet.

As of September 3, the Northeast Pacific had produced 15 named storms and six hurricanes, well above the norm for that point in the season. The Atlantic basin, meanwhile, laboring under unfavorable wind shear conditions, had produced just five named storms and no hurricanes. El Niño typically enhances hurricane activity in the eastern and central Pacific basins because of the unusually warm water temperatures it brings to those parts of the ocean. It tends to suppress hurricane activity in the Atlantic basin by shifting large-scale circulation patterns in a way that makes it harder to sustain storms there.

At 1:14 p.m. Pacific Daylight Time (20:14 Universal Time) on September 1, NASA’s EPIC (Earth Polychromatic Imaging Camera) on the DSCOVR (Deep Space Climate Observatory) satellite captured an image of three tropical cyclones churning simultaneously in the Pacific, along with one in the Atlantic. A band of clouds and thunderstorms associated with the Intertropical Convergence Zone (ITCZ) is visible to the south of the storms. The spacecraft was nearly 1 million miles from Earth and just shy of 93 million miles from the Sun when the image was acquired.

The trio of storms in the Pacific were Lowell, Karina, and Marie. Of the three, Lowell became the strongest, with winds reaching category 5 strength for several hours on September 2. Around the same time, Karina, spinning a few thousand kilometers to the east, achieved category 4 strength, a rare case of category 4 and 5 hurricanes occurring simultaneously in the area. Marie, spinning southwest of Baja California, was still a tropical storm when the image was acquired but was strengthening as it moved northwest.

In the Atlantic, Tropical Storm Edouard was visible to EPIC over Louisiana and Texas, shortly after the short-lived storm made landfall. It brought torrential rains and strong winds that downed trees and power lines. Some areas received 15 to 24 inches (38 to 61 centimeters) of rain, according to National Weather Service meteorologists.

As of September 3, the Atlantic basin’s total accumulated cyclone energy (ACE) index was 4.4, about 9 percent of normal for that date, according to statistics compiled by Colorado State University meteorologists. Meanwhile, the Northeast Pacific basin’s ACE was 130, about 50 percent above normal. The ACE index incorporates both the intensity and longevity of storms, making it easier to compare individual storms and seasons.

Several NASA Earth-observing platforms provide data that can aid in emergency preparedness before landfall and damage assessment and response afterward. Use the “Events” tab on NASA’s Worldview browser to track current hurricanes and explore related NASA data products.

NASA Earth Observatory image by Lauren Dauphin, using data from DSCOVR EPIC. Story by Adam Voiland.

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