NASA’s B777 Gets New Coat of Paint

NASA’s B777 Gets New Coat of Paint

A large airplane flies in the sky. It is painted white (the first two-thirds) and blue (the last one-third), with the NASA "worm" logo on the side and wing. The NASA "meatball" logo is on the tail. Fluffy white clouds line the air below the plane.
NASA’s Boeing 777 returns to the agency’s Langley Research Center after receiving a new paint scheme.
NASA/James Blair

NASA’s Boeing 777 shows off a new paint job in this Aug. 11, 2026, photo. The B777 was acquired to replace and extend the capabilities of the NASA DC-8, which was retired in 2024.

The B777, set to begin operations from NASA’s Langley Research Center in Hampton, Virginia in 2027, will be a unique flying laboratory with global reach enabling data collection for NASA projects to include sensor development, satellite sensor calibration, data product validation, and field studies to better understand Earth system processes to improve models and decision-making.

Image credit: NASA/James Blair

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NASA Glenn’s Legacy Forged Through Decades of Flight Research

NASA Glenn’s Legacy Forged Through Decades of Flight Research

A pilot steps on a metal ladder to get onto a small, one-seater airplane. The NACA hangar is in background
William “Bill” Swann, one of the first-generation pilots at the National Advisory Committee for Aeronautics’ Flight Propulsion Research Laboratory (predecessor to NASA’s Glenn Research Center in Cleveland), prepares to board a McDonnell F2H-2B airplane on Nov. 6, 1956.
Credit: NASA

Many of NASA’s most important aerospace breakthroughs that began in the laboratory were ultimately proven in the sky. For decades, experts at NASA’s Glenn Research Center in Cleveland conducted flight tests — piloting aircraft into targeted environments such as icing clouds and carefully defined atmospheric routes. This approach allowed them to collect measurements directly in flight, providing critical data that linked laboratory theories to practical performance. 

The center’s flight research dates to the 1940s, when NASA Glenn was known as the Aircraft Engine Research Laboratory for the National Advisory Committee for Aeronautics, NASA’s predecessor agency. During World War II, engineers and pilots worked to improve aircraft performance and increase high-altitude reliability. In the mid-to-late-1940s, flight research helped make early jet and ramjet engines practical. Later, Glenn’s flight programs helped improve the efficiency and environmental performance of aircraft engines — primarily conventional jet engines. 

Behind those early flight programs was a pioneering group of pilots who helped establish NASA Glenn’s reputation for airborne research. The center’s first generation of pilots, including Howard Lilly, Joseph Walker, William Swann, and William “Ed” Gough, helped lay the groundwork for more than two dozen other Glenn pilots, including future astronauts Neil A. Armstrong and Fred Haise. 

Together with Glenn’s researchers, engineers, and support staff, these pilots established airborne research capabilities that NASA continues to rely on today. Their work demonstrated how flight testing could bridge the gap between laboratory research and real-world performance. 

“These missions transformed aircraft into flying laboratories,” said Mark Russell, a NASA safety officer and pilot who served as the former acting chief of Aircraft Operations at Glenn. “They bridged the gap between ground testing and full-scale flight, proving the measurements needed to connect theory with performance. The testing also helped validate technologies and procedures later used aboard spacecraft and orbital missions.” 

Research workhorses 

From the start, NASA put its aircraft to work on a wide range of research challenges. 

For decades, NASA Glenn aircraft have been used to study in-flight icing hazards, collecting data that has helped make commercial aviation safer. For nearly 40 years, NASA Glenn’s De Havilland DHC-6 Twin Otter served as the center’s workhorse for icing research, gathering data that helped shape modern aviation safety standards. 

Two men in flight suits stand in front of a small aircraft painted white and blue. Behind it is an aircraft hangar with the NASA logo at the top.
Pilot Richard Ranaudo, left, and engineer Thomas Ratvasky with the De Havilland Twin Otter at NASA’s Glenn (then Lewis) Research Center in Cleveland on Feb. 23, 1993. The aircraft helped advance global aviation safety by defining the precise atmospheric physics of supercooled clouds and validating critical modern technologies used to predict, detect, and prevent in-flight icing hazards.
Credit: NASA/Tom Jares

Beyond improving aviation safety, Glenn’s flight research also explored new propulsion technologies that could transform the future of flight. Today, researchers are exploring hydrogen as an aviation fuel. But NASA Glenn helped show its potential viability decades ago using its Martin B-57B Canberra aircraft. After developing a hydrogen fuel system for the B-57B, a team tested it safely from February to April 1957. The flights showed the system’s reliable operation and advanced efficiency, marking a major milestone in aviation technology.  

Flight testing also supported technologies destined for use beyond Earth, helping researchers evaluate hardware under conditions that closely resembled space. Beginning in 1963, the center began a program to test and measure how well solar cells worked under conditions similar to those in space. Using specially modified airplanes, including Learjets, NASA conducted flights to help recreate some of the sunlight and atmospheric conditions that solar cells would experience outside Earth’s atmosphere. The program lasted decades, supporting space technology calibration through numerous high-altitude flights and adapting to newer aircraft over time. 

Researchers later applied these airborne capabilities to environmental science, extending their value beyond aviation and space technology. Using the Twin Otter and S-3B Viking over the Great Lakes, researchers tracked harmful algal blooms on Lake Erie by measuring changes in water color and composition. The data improved satellite systems used to monitor water quality and ecosystem health.  

Glenn’s research aircraft also played an important role in preparing technologies and experiments for spaceflight through microgravity testing. NASA Glenn advanced microgravity research through in-flight testing using specially modified aircraft, such as its DC-9, to create short periods of weightlessness during parabolic maneuvers. These flights allowed researchers to study how fluids, combustion, materials, and experimental equipment behaved in near-zero gravity before experiments were conducted in space.  

Inside the bed of an aircraft with no seating, three people in gray flight suits hang onto the sides of the plane to gain balance in the microgravity atmosphere. To the left, a flight research staff member assists. Researchers make their way to two small tables that contain test hardware.
NASA’s Glenn (then Lewis) Research Center in Cleveland conducted microgravity research using the DC-9 airplane. Pictured, back to front, John Yaniec, Mike Mahn, Michael Capelety, and Susan Motil conduct microgravity research during a flight on July 10, 1996.
Credit: NASA/Quentin Schwinn

Recent breakthroughs 

Other significant accomplishments enabled by Glenn’s flight research include supporting the development and testing of sustainable aviation technologies, including research related to more fuel-efficient engines and sustainable aviation fuels, and advancing in-flight instrumentation and measurement techniques used across aeronautics research. 

In 2024, Glenn’s Flight Operations participated in an optical communications study using the center’s Pilatus PC-12 NG aircraft. This mission successfully demonstrated the ability to transmit large volumes of data through a laser communication system across NASA’s legacy infrastructure. The work contributed to NASA’s broader effort to advance optical communications for future missions. NASA further tested optical communications on the Artemis II mission and effectively transmitted substantial amounts of data from the Orion capsule to multiple ground stations over the course of the 10-day journey.  

A team at NASA’s Glenn Research Center in Cleveland streamed 4K video footage from a Pilatus airplane to the International Space Station and back for the first time using optical, or laser, communications. Pictured on June 13, 2024, left to right, James Demers, Adam Wroblewski, Shaun McKeehan, and Kurt Blakenship.
Credit: NASA/Sara Lowthian-Hanna

As NASA’s flight research enterprise evolved, the agency also restructured how it manages its research aircraft. In October 2025, NASA streamlined its aircraft flight operations, relocating its aircraft from Glenn to NASA’s Armstrong Flight Research Center in Edwards, California. NASA Glenn continues its important icing and propulsion research and communications technology development in collaboration with Armstrong.  

From its historical roots in wartime engine development to modern work on aircraft safety, Glenn’s airborne research has consistently moved innovative ideas from the laboratory to real-world application. For more than eight decades, NASA Glenn has transformed ideas first proven in the laboratory into innovations validated in the sky — a legacy that continues to shape the future of aviation and space exploration. 

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Heather Baeslack

APOD: 2026 August 18 – Perseids from Perseus

APOD: 2026 August 18 – Perseids from Perseus

APOD

Astronomy Picture of the Day

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

A starfield is bounded by trees on three sides and a pond on the bottom. Amongst the stars are many streaks of light appearing to emanate from a place on the sky just above a foreground bridge.

Perseids from Perseus

Explanation: This was a good year for the Perseids meteor shower. A key reason was the Moon was absent from lighting up Earth’s night sky so that more meteors were visible than usual. Where was the Moon? It was busy visiting the Sun. Near the Perseids peak, the Moon moved directly in front of the Sun and created a total solar eclipse visible from Greenland and Spain. The Perseids occur when the Earth collides with a stream of Sun-orbiting debris cast off by Comet Swift-Tuttle. Perseid meteors, although typically only the size of a sand grain, tend to be fast and bright because Swift-Tuttle’s debris orbits the Sun in a direction partly opposite Earth’s orbital motion. In the featured image compilation, accumulated over several nights from Jizerka in the Czech Republic, the Perseids meteor streaks can be traced back to a single location on the sky — its radiant in Perseus.

Gallery: 
Perseids Meteor Shower of 2026
Tomorrow’s picture: open space

Date August 18, 2026
Credit Jakub Kuřák
Authors & editors: Robert Nemiroff, Jerry Bonnell, Cecilia Chirenti, Keighley Rockcliffe
A service of: ASD at NASA / GSFC,
NASA Science Activation & Michigan Tech. U.

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Lala Batters Hawaii

Lala Batters Hawaii




August 16, 2026
August 15, 2026

The spiraling clouds of a tropical storm are centered near the Hawaiian island of Kauaʻi.
The spiraling clouds of a tropical storm are centered near the Hawaiian island of Kauaʻi.
NASA Earth Observatory / Lauren Dauphin

The spiraling clouds of a hurricane appear near the Hawaiian Islands. Its eye is just south of the Island of Hawaiʻi.
The spiraling clouds of a hurricane appear near the Hawaiian Islands. Its eye is just south of the Island of Hawaiʻi.
NASA Earth Observatory / Lauren Dauphin

The spiraling clouds of a tropical storm are centered near the Hawaiian island of Kauaʻi.
The spiraling clouds of a tropical storm are centered near the Hawaiian island of Kauaʻi.
NASA Earth Observatory / Lauren Dauphin

The spiraling clouds of a hurricane appear near the Hawaiian Islands. Its eye is just south of the Island of Hawaiʻi.
The spiraling clouds of a hurricane appear near the Hawaiian Islands. Its eye is just south of the Island of Hawaiʻi.
NASA Earth Observatory / Lauren Dauphin


August 16, 2026

August 15, 2026


Lala skirts south of the Island of Hawaiʻi as a category 1 hurricane in the right image, acquired by the VIIRS (Visible Infrared Imaging Radiometer Suite) on the Suomi NPP satellite on August 15, 2026, at about 1:45 p.m. Hawaii Standard Time (23:45 Universal Time). The storm decreased in intensity while tracking northwest and was a tropical storm when the VIIRS on the NOAA-20 satellite captured the left image about 24 hours later. NASA Earth Observatory images by Lauren Dauphin.

The Island of Hawaiʻi narrowly avoided a direct landfall by Hurricane Lala in mid-August 2026. The storm nonetheless delivered serious damage as it passed just south of the island on August 15 (above, right) as a category 1 storm on the Saffir-Simpson wind scale.

Lala brought rainfall totals exceeding 20 inches (50 centimeters) to parts of the island, causing flash flooding and ongoing mudflow risks. The highest rainfall total for the storm—43.55 inches (110.6 centimeters) as of the morning of August 17—was recorded at Laupāhoehoe, on the coast northwest of Hilo. Lala downed trees, damaged bridges, and knocked homes off their foundations. Coastal areas were pummeled by large waves, while the summit of Mauna Kea, over 13,000 feet (4,000 meters) above sea level, experienced blizzard conditions.

By early afternoon on August 16, when the other image (left) was acquired, the storm had tracked northwest, roughly parallel to the island chain, and was southwest of Kauaʻi. Lala had decreased in intensity to a tropical storm, with sustained winds of 65 miles (105 kilometers) per hour, according to the National Hurricane Center.

While the Island of Hawaiʻi took the brunt of the storm, other islands also saw destructive effects. Strong winds caused widespread power outages, with more than 220,000 customers statewide without power as of the afternoon of August 16, according to news reports. Across the islands, wind and rain damaged infrastructure, and floodwaters and debris rendered roads impassable.

It has been an active tropical cyclone season in the Eastern Pacific so far in 2026, meteorologists note, consistent with what scientists expect during an El Niño, which has been underway as of mid-June. Warm water in the equatorial Pacific—the hallmark of El Niño—and the moisture and energy it transfers to the atmosphere help fuel nascent tropical storms. Lack of wind shear, another typical El Niño pattern in this region, also encourages tropical storms to develop and strengthen. The Atlantic hurricane season, in contrast, has been relatively calm, as greater wind shear over the Atlantic Ocean and Caribbean Sea during an El Niño inhibits hurricane formation by dissipating the upward motion of heat.

NASA Earth Observatory images by Lauren Dauphin, using VIIRS data from NASA EOSDIS LANCE, GIBS/Worldview, and the Joint Polar Satellite System (JPSS). Story by Lindsey Doermann.

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Curiosity Blog, Sols 4975-4981: Happy 14th Landing Anniversary

Curiosity Blog, Sols 4975-4981: Happy 14th Landing Anniversary

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Curiosity Blog, Sols 4975-4981: Happy 14th Landing Anniversary

A black-and-white image from the Curiosity rover on Mars. The rover's robotic arm and instrument turret are extended downward toward a large, flat, cracked rock on the Martian surface. Portions of the rover's wheels are visible on the left and right edges, with a barren, rocky landscape and distant hills in the background.
NASA’s Mars rover Curiosity acquired this image, of its onboard APXS instrument measuring target “Tunas Khasa,” using its Front Hazard Avoidance Camera (Front Hazcam). Curiosity captured the image on Sol 4976 — Martian day 4,976 of the Mars Science Laboratory mission — at 03:01:56 UTC.
NASA/JPL-Caltech

By Susanne P. Schwenzer, Professor of Planetary Mineralogy at The Open University, UK

Earth planning date: Friday, Aug. 7, 2026

This week was very special for the Curiosity team here on Earth as we celebrated the 14th landing anniversary. I still remember watching the buildup to the entry phase on “Eyes on the Solar System” and then I don’t remember much until I heard the words, “We are safe on Mars.” I was just too tense and nervous, but I love to re-live the moments each year when we celebrate another (Earth) year on Mars. If you want to remember it all, you can go to NASA’s interactive tool “Eyes on the Solar System” use the menu and find the Mars Science Laboratory Rover in the list of spacecraft. Curiosity launched Nov. 26, 2011, 15:02 UTC; you can wind back the clock to that day as the spacecraft leaves Earth and follow as it gradually makes its way to Martian orbit, where it meets Mars at just the right moment. Curiosity landed Aug. 6, 2012, 05:17 UTC. The big moment to me, though, is to see the joy and celebrations in the control room after landing. I have watched this video more times than I can count; it’s just too good to not remember: Curiosity Has Landed – NASA Science.

But what did we do in that very special week that marked the transition from year 14 to year 15? Of course it was business as usual for the rover while many of us exchanged memories and also marveled at what we have found to date. If you are interested what exactly Curiosity did at the moment in time that marked the landing anniversary, we’ve got you covered — with the help of the science and engineering team at JPL in Pasadena, I can tell you that this was on Sol 4976 at 19:47 LMST on Mars, and at that very moment the rover’s arm was deployed at the target “Tunas Khasa” doing an APXS measurement.

The rover continued its way up Mount Sharp investigating the different layers of rock along the way. This climb can be quite steep and coming into Monday’s plan was no different. At one point last Friday the rover’s tilt was 24 degrees. But the engineers know exactly what Curiosity can do, so we arrived safely at our planned location coming into Monday. At this first stop of the week, the APXS measured “Tunas Khasa” and “Villarrica,” which were also imaged with our Mars Hand Lens Imager (MAHLI). More chemistry came from ChemCam investigating the targets “Lago Rupanco” and “Chulipa Punta.” ChemCam also used its Remote Micro Imager to acquire high-resolution images of targets of interest. We are specifically looking for the cross-bedding, a term geologists use to describe rock layers that tilt and intersect each other, and how the different layers of rock relate to each other. Mastcam had five different mosaics in the plan, investigating targets in the nearfield and looking into the distance, too. The targets range from layers of rocks in the walls that make up the buttes around the rover to bedrock targets in the nearfield. “La Linea” is a surface that displays signs of erosion, and “Tiraque” gives insights into the layering of the bedrock, just to name two of the Mastcam targets. Of course, the future drive direction and the future workspace​ were also imaged after the drive. In addition to the science, there were some “housekeeping” activities in the plan, too. Those were a SAM column-cleaning activity and MAHLI images of the REM UV sensor. It’s important to keep on top of these things, too!

The 46-foot (14-meter) drive put us into the perfect position in front of one of those very special places, where not only two different rock layers meet, but also where cross-bedded rocks are truncated by other layers. It is those special places that allow us – one by one – to put the pieces of the puzzle together, showing what happened here billions of years ago. One thing is clear: it involved wind, lots of wind, but also some water. As this location is an exceptionally interesting place, we will stay here through Monday and spend two planning cycles at this location.

On Friday we planned two APXS on a bedrock block in front of us – keeping in mind two others for our colleagues to plan on Monday. The two targets are “Salar de Gorbea” and “Uriondo.” MAHLI documents those two, but also has a mosaic in the plan that is one of the largest I have ever seen. It’s on the target “Tres Morros,” which is an excellent example on how exactly those different rock layers meet. The team can’t wait to see the high-resolution MAHLI images and inspect every single detail visible in them. Mastcam also was very busy, investigating representative outcrops in the nearfield and further away. Targets to especially look out for are “Laguna Del Eulogio” and “Laguna de Pozuelo,” as they image outcrops related to the changes in the rock layers and further ahead on a butte called Mishe Mokwa. You might remember the latter from many mentions previously as we were driving along and around it, and using repeated images to get stereo views, but also understand different aspects of the stratigraphy (the way rocks are layered). ChemCam looks at target “Rio Tranquilo,” which is a nodular target, possibly giving insights into the water-related part of the environments that formed those rocks. The other ChemCam target is “Rio Juncalito,” which is a cross-bedded target. ChemCam also has two RMIs in the plan, one targeting forward toward Valle Grande and the other looking at Mishe Mokwa.

Both plans contain a rich set of environmental monitoring. There are many dust-devil surveys alongside measurements of the atmospheric opacity and wind monitoring. We are also looking for clouds, and of course the RAD instrument is actively measuring the radiation environment. It rarely gets a mention here, because it sits quietly in its place within the rover, looking out to the sky and monitoring the radiation — for all those 14 years, and in fact a little longer, because it was the first instrument to be switched on after launch and already started its monitoring during the cruise phase to Mars.

Happy 14th Landing Anniversary, Curiosity!

A rover sits on the hilly, orange Martian surface beneath a flat grey sky, surrounded by chunks of rock.
NASA’s Curiosity rover at the base of Mount Sharp
NASA/JPL-Caltech/MSSS

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Last Updated
Aug 17, 2026

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