Introduction

On November 16, 2025, the Sentinel-6B satellite launched from Vandenberg Space Force Base (VSFB) in California. The mission is a partnership between NASA, the National Oceanic and Atmospheric Administration (NOAA), and several European partners – the European Space Agency (ESA), the European Organisation for the Exploitation of Meteorological Satellites (EUMETSAT), the French Centre National d’Études Spatiales (CNES), and the European Commission. Its objective is to continue collecting data to extend the ocean height record, which was started in 1992 with the U.S./French TOPEX/Poseidon satellite mission. During the past three decades, NASA and its partners have operated a satellite in the same orbit, precisely tracking the height of the oceans across the globe, once every 10 days.

Sentinel-6B took to the skies almost five years to the day after its twin, Sentinel-6A, which launched November 20, 2020, also from VSFB, and was renamed Sentinel–6 Michael Freilich, honoring the former head of NASA’s Earth Science Division – see The Editor’s Corner [March–April 2020, 32:1, 1–2]. Together, the two missions comprise the international Sentinel-6/Jason – Continuity of Service (CS) mission, which will provide continuity with past missions from TOPEX/Poseidon through Jason-3. Sentinel-6B will continue to measure sea level to about one inch (2.5 cm), extend the record of atmospheric temperatures, and continue sea level observations through the end of the 2020s.

The article that follows briefly introduces Sentinel-6B’s payload (which is the same as Sentinel–6 Michael Freilich). It then describes the planned science applications of the mission, followed by a brief conclusion.

Sentinel-6B Payload

The Sentinel-6B satellite carries several instruments to support the mission’s science goals – see Figure 1. A Radar Altimeter bounces signals off the ocean surface to determine the distance to the ocean. An Advanced Microwave Radiometer (AMR) retrieves the amount of water vapor between the satellite and ocean, which affects the travel speed of radar pulses, providing a critical correction to the distance measured by the radar. Other onboard instruments are used to precisely determine the satellite’s position [e.g., Doppler Orbitography by Radiopositioning Integrated on Satellite (DORIS) and Laser Retroreflector Array]. The height of the ocean surface can be calculated by combining the satellite’s position with the distance to the ocean. In addition, S- and X-band antennas perform data downlinks, and a solar array supplies power.

Beyond these instruments, Sentinel-6B contains Global Navigation Satellite System Radio Occultation (GNSS-RO) instrument that will aid with weather prediction. Observations made between the spacecraft instrument and other GNSS satellites as they disappear over Earth’s limb, or horizon, will provide detailed information about variations in the layers of the atmosphere. This information will contribute to computer models that predict the weather and enhance forecasting capabilities.

Sentinel-6B Science

The subsections that follow give a short preview of Sentinel-6B’s science capabilities, which are identical to those of Sentinel-6 Michael Freilich and similar – albeit enhanced – to the capabilities of previous satellite altimetry missions.

Measuring Ocean Height

Ocean height is a critical measurement because it provides a host of information about the movement of surface currents, transfer of energy around the planet, and an early warning system for large-scale climate phenomena, like El Niño–Southern Oscillation (ENSO) – see further discussion of ENSO below. Satellites obtain this data using altimeters, which send a radar pulse to the ocean surface every second and measure the time it takes to return. Pairing these data with the satellite’s precise location provides a measure of the height of the ocean water with an accuracy of within a few centimeters.

But the simplicity of the measurement belies the volumes of information that can be gleaned from the height of the oceans. As water moves from one place to another, it tilts the surface of the ocean, and by measuring this tilt the sea level satellites allow scientists to calculate ocean currents – see Figure 2.

Tracking the Expansion and Contraction of Water in the Ocean

Ocean height data also provide information about ocean water temperature. Since water expands as it warms, a warm patch of ocean measures several inches taller than a cold patch – see Figure 3. Ocean height measurements thus can be used to reveal how the ocean stores and redistributes heat and energy, which are key drivers of Earth’s climate.

By observing ocean heights, Sentinel-6B will help improve forecasters’ ability to predict storm intensity and scientists’ ability to track long-term trends in heat storage. Information on ocean height also outlines ocean currents, eddies, and tides, which helps scientists understand how heat, nutrients, carbon, and energy are transported around Earth. These observations are essential for understanding Earth’s energy balance, ocean circulation, and the role of the ocean in shaping weather and climate patterns.

Using Ocean Height Measurements to Track ENSO

The movement of heat within the ocean is linked to weather and climate conditions across the globe. For reasons not completely understood, the waters of the Pacific Ocean experience a periodic fluctuation between warm and cool in the eastern tropical Pacific; this cycle is called ENSO. During an El Niño event in the Pacific Ocean, unusually warm water (which is visible in the satellite data as higher than normal sea levels) builds up along the equator in the east. The pool of warm water shifts rainfall patterns across the United States and Canada. This change is telescoped around the globe, altering normal weather patterns. Conversely, La Niña events develop when cooler waters accumulate along the eastern Pacific (and hence, lower than normal sea levels). In this way, the satellite observations of sea level help scientists and forecasters better see how the ocean is changing and the type of weather conditions to expect in the coming months – see Figure 4.

Higher sea levels usually mean warmer waters, not just at the surface, but over a range of depths. This means that high sea levels can also herald rapidly intensifying storms. Meteorologists can use this information when tracking tropical storms that gain energy from warm patches of ocean water and intensify into hurricanes – often rapidly.

Monitoring Ocean Changes

Sentinel-6B can also monitor changes in sea level. Over 90% of the heat trapped by the Earth is stored in the oceans. That heat warms the water, which takes up more space and accounts for about one-third of the observed global rise in sea level. The remainder is driven by melting glaciers and ice sheets, which add water to the oceans as well. The result is a long-term rise in sea level by more than 10 cm (4 in) since the early 1990s, when TOPEX/Poseidon was launched.

A record of global mean sea level change for the past three decades reveals an annual oscillation that reflects the natural movement of water between the ocean and the land, much like the heartbeat of the planet – see Figure 5. The rate of rise is not steady. The change in sea level in the 1990s was less than half the rate of rise in the most recent decade.

Conclusion

This unbroken record of sea level change stands as a crowning achievement to the accuracy, stability, and consistency of a series of satellite missions across more than three decades. This approach remains one of the most successful international collaborations to study our ever-changing Earth from space, and the launch of Sentinel-6B will stretch the record to nearly 40 years. With a vibrant international community of several hundred scientists and expert users, the discoveries made, and the value created by these observations will no doubt extend through 2030 and beyond. Although Sentinel-6B is nearly identical to its predecessor, a broad community of scientists, forecasters, operational users, and policymakers anxiously await its observations and the discoveries and utility they will bring through the remainder of this decade.

Joshua Willis
NASA/Jet Propulsion Laboratory
joshua.k.willis@jpl.nasa.gov

Severine Fournier
NASA/Jet Propulsion Laboratory
severine.fournier@jpl.nasa.gov

Teams at NASA’s Kennedy Space Center in Florida spent 2025 preparing the launch vehicle and its powerhouse SLS (Space Launch System) rocket to launch four astronauts around the Moon for Artemis II in early 2026. The center also celebrated milestones by conducting science experiments at the International Space Station to studying the Sun’s solar wind impacts on Earth to traveling to Mars in hopes of one day exploring the Red Planet in person.

JANUARY
NASA Kennedy Marks New Chapter for Florida Space Industry 

Kennedy Space Center Director Janet Petro and charter members of the Florida University Space Research Consortium sign a memorandum of understanding in research and development to assist with missions and contribute to NASA’s Moon to Mars exploration approach. 

Firefly Launches Blue Ghost Mission One 

Firefly Aerospace launched Blue Ghost Mission One lunar lander with a suite of NASA scientific instruments on January 15, from Launch Complex 39A at NASA Kennedy. The lander and instruments landed March 2 on the Moon. 

FEBRUARY
Intuitive Machines Launches to the Moon

Intuitive Machines’ IM-2 Nova C lunar lander launched Feb. 26 from Launch Complex 39A, carrying NASA science and technology demonstrations to the Mons Mouton region of the Moon. IM-2 reached the surface of the Moon on March 6. 

MARCH
NASA’s SpaceX Crew-10 Launch

NASA astronauts Anne McClain and Nicole Ayers, JAXA (Japan Aerospace Exploration Agency) Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov launched March 14 from Launch Complex 39A to the International Space Station for a five-month science mission. 

NASA’s SPHEREx, PUNCH Missions Launch 

A SpaceX Falcon 9 rocket launched on March 11, from Space Launch Complex 4 East at Vandenberg Space Force Base in California carrying NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer) and PUNCH (Polarimeter to Unify the Corona and Heliosphere) missions. NASA’s Launch Services Program, based at NASA Kennedy managed the launch service for SPHEREx.

NASA’s SpaceX Crew-9 Returns 

NASA astronauts Nick Hague, Suni Williams, and Butch Wilmore were greeted by dolphins and recovery teams after their SpaceX Dragon spacecraft splashed down on March 18, off the coast of Tallahassee, Florida following their long-duration mission at the International Space Station. 

NASA Causeway Bridge Opens 

The Florida Department of Transportation opened the westbound portion of the NASA Causeway Bridge on March 19, completing construction in both directions spanning the Indian River Lagoon and connecting NASA Kennedy and Cape Canaveral Space Force Station to the mainland. 

NASA Artemis Teams Complete URT-12 

Teams from NASA and the Department of War train during a week-long Underway Recovery Test-12 in March off the coast of California for Artemis II test flight crewmembers and the Orion spacecraft. The series of tests demonstrate and evaluate the processes, procedures, and hardware used in recovery operations for crewed lunar missions.

APRIL  
NASA’s SpaceX 32nd Commercial Resupply Mission 

A SpaceX Falcon 9 rocket and a Dragon spacecraft carrying nearly 6,700 pounds of scientific investigations, food, supplies, and equipment launched on April 21 from Launch Complex 39A to the International Space Station. 

JULY
Artemis III Begins Processing

NASA’s Artemis III SLS engine section and boat-tail made the journey from the Space Systems Processing Facility at NASA Kennedy to the spaceport’s Vehicle Assembly Building in July to complete integration and check-out testing. Beginning with the Artemis III hardware, NASA moved certain operations to NASA Kennedy to streamline the manufacturing process and enable simultaneous production operations of two core stages.

AUGUST 
NASA’s SpaceX Crew-11 Launches 

NASA astronauts Zena Cardman and Mike Fincke, JAXA (Japan Aerospace Exploration Agency) astronaut Kimiya Yui, and Roscosmos cosmonaut Oleg Platonov launched aboard a SpaceX Dragon spacecraft and its Falcon 9 rocket on Aug. 1 from Launch Complex 39A bound for a long-duration mission to the International Space Station. 

NASA’s SpaceX Crew-10 Returns 

NASA astronauts Anne McClain and Nicole Ayers, JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov became the first Commercial Crew to splash down in the Pacific Ocean off the coast of California on Aug. 9, completing their nearly five-month mission at the orbiting outpost as part of the agency’s Commercial Crew Program. 

NASA’s SpaceX 33rd Commercial Resupply Mission 

A SpaceX Falcon 9 launched the company’s Dragon spacecraft carrying more than 5,000 pounds of food, crew supplies, science investigations, spacewalk equipment, and more to the space station on Aug. 24 from Launch Complex 39A. 

Orion Tested, Stacked With Hardware

Teams transported NASA’s Orion spacecraft from Kennedy’s Multi-Payload Processing Facility to the Launch Abort System Facility in August where crews integrated the 44-foot-tall launch abort system. The Orion spacecraft will send NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen around the Moon for the Artemis II mission in early 2026. The launch abort system is designed to carry the crew to safety in the event of an emergency atop the SLS.

SEPTEMBER
NASA Launches IMAP Mission

NASA’s IMAP (Interstellar Mapping and Acceleration Probe) launched from Launch Complex 39A on Sept. 24, to help researchers better understand the boundary of the heliosphere, a huge bubble created by the Sun surrounding and protecting our solar system.

NASA’s Northrop Grumman Commercial Resupply Mission 

A Northrop Grumman Cygnus XL spacecraft atop a SpaceX Falcon 9 rocket lifted off from Launch Complex 39A to the International Space Station delivering NASA science investigations, supplies, and equipment as part of the agency’s partnership to resupply the orbiting laboratory.  

OCTOBER
Orion Integrated With SLS Rocket

Teams stacked NASA’s Orion spacecraft with its launch abort system on the agency’s SLS rocket in High Bay 3 of the Vehicle Assembly Building at NASA Kennedy on Oct. 20 for the agency’s Artemis II mission. Teams will begin conducting a series of verification tests ahead of rolling out the integrated SLS rocket to Launch Complex 39B for the wet dress rehearsal.

NOVEMBER
NASA’s ESCAPADE Begins Journey to Mars

NASA’s ESCAPADE (Escape and Plasma Acceleration and Dynamics Explorers) twin spacecraft launched aboard Blue Origin’s New Glenn rocket on Nov. 13 from Launch Complex 36 at Cape Canaveral Space Force Station. Its twin orbiters will take simultaneous observations from different locations around Mars to reveal how the solar wind interacts with Mars’ magnetic environment and how this interaction drives the planet’s atmospheric escape.

NASA, European Partners Launch Sea Satellite

A SpaceX Falcon 9 rocket carrying the U.S.-European Sentinel-6B satellite launched at Nov. 16 from Space Launch Complex 4 East at Vandenberg Space Force Base in California. Sentinel-6B will observe Earth’s ocean, measuring sea levels to improve weather forecasts and flood predictions, safeguard public safety, benefit commercial industry, and protect coastal infrastructure.

DECEMBER

NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and CSA astronaut Jeremy Hansen participated in a dry dress rehearsal at NASA Kennedy on Dec. 20 to mimic launch day operations for the Artemis II launch. The crew donned their spacesuits, exited the Neil A. Operations and Checkout Building, and took the journey to the Vehicle Assembly Building, up the mobile launcher to the crew access arm, and entered the Orion spacecraft that will take them around the Moon and back to Earth.

NASA’s James Webb Space Telescope captured two nearby dwarf galaxies interacting with each other in this image released on Dec. 2, 2025. Dwarf galaxies can give us insights into galaxies in the early universe, which were thought to have less mass than galaxies like the Milky Way, and also contain a lot of gas, relatively few stars, and typically have small amounts of elements heavier than helium. Observing dwarf galaxies merge can tell us how galaxies billions of years ago might have grown and evolved.

Read more about this cosmic pair.

Image credit: ESA/Webb, NASA & CSA, A. Adamo (Stockholm University), G. Bortolini, and the FEAST JWST team

In 2025, NASA’s Armstrong Flight Research Center in Edwards, California, advanced work across aeronautics, Earth science, exploration technologies, and emerging aviation systems, reinforcing its role as one of the agency’s primary test sites for aeronautics research. From early concept evaluations to full flight test campaigns, teams enhanced measurement tools, refined safety systems, and generated data that supported missions across NASA. Operating from the Mojave Desert, NASA Armstrong continued applying engineering design with real-world performance, carrying forward research that informs how aircraft operate today and how new systems may function in the future.

The year’s progress also reflects the people behind the work – engineers, technicians, pilots, operators, and mission support staff who navigate complex tests and ensure each mission advances safely and deliberately. Their efforts strengthened partnerships with industry, small businesses, and universities while expanding opportunities for students and early career professionals. Together they sustained NASA Armstrong’s long-standing identity as a center where innovation is proven in flight and where research helps chart the course for future aviation and exploration.

“We executed our mission work safely, including flight of the first piloted NASA X-plane in decades, while under challenging conditions,” said Brad Flick, center director of NASA Armstrong. “It tells me our people embrace the work we do and are willing to maintain high levels of professionalism while enduring personal stress and uncertainty. It’s a testimony to the dedication of our NASA and contractor workforce.”

Teams continued advancing key projects, supporting partners, and generating data that contributes to NASA’s broader mission.

Quiet supersonic flight and the Quesst mission

NASA Armstrong continued its quiet supersonic research, completing a series of activities in support of NASA’s Quesst mission. On the X-59 quiet supersonic research aircraft, the team performed electromagnetic interference tests and ran engine checks to prepare the aircraft for taxi tests. The Schlieren, Airborne Measurements, and Range Operations for Quesst (SCHAMROQ) team completed aircraft integration and shock-sensing probe calibration flights, refining the tools needed to characterize shock waves from the X-59. These efforts supported the aircraft’s progression toward its first flight on Oct. 28, marking a historic milestone and the beginning of its transition to NASA Armstrong for continued testing.

The center’s Commercial Supersonic Technology (CST) team also conducted airborne validation flights using NASA F-15s, confirming measurement systems essential for Quesst’s next research phase. Together, this work forms the technical backbone for upcoming community response studies, where NASA will evaluate whether quieter supersonic thumps could support future commercial applications.

• The X-59 team completed electromagnetic interference testing on the aircraft, verifying system performance and confirming that all its systems could reliably operate together.
• NASA’s X-59 engine testing concluded with a maximum afterburner test that demonstrated the engine’s ability to generate the thrust required for supersonic flight.
• Engineers conducted engine speed-hold evaluations to assess how the X-59’s engine responds under sustained throttle conditions, generating data used to refine control settings for upcoming flight profiles.
• NASA Armstrong’s SCHAMROQ team calibrated a second shock-sensing probe to expand measurement capability for future quiet supersonic flight research.
• NASA Armstrong’s CST team validated the tools that will gather airborne data in support the second phase of the agency’s Quesst mission.
• NASA’s X-59 team advanced preparations on the aircraft through taxi tests, ensuring aircraft handling systems performed correctly ahead of its first flight.
• NASA Armstrong’s photo and video team documented X-59 taxi tests as the aircraft moved under its own power for the first time.
• The X-59 team evaluated braking, steering, and integrated systems performance after the completion of the aircraft’s low-speed taxi tests marking one of the final steps before flight.
• NASA Armstrong teams advanced the X-59 toward first flight by prioritizing safety at every step, completing checks, evaluations, and system verifications to ensure the aircraft was ready when the team was confident it could move forward.
• NASA and the Lockheed Martin contractor team completed the X-59’s historic first flight, delivering the aircraft to NASA Armstrong for the start of its next phase of research.

Ultra-efficient and high-speed aircraft research

Across aeronautics programs, Armstrong supported work that strengthens NASA’s ability to study sustainable, efficient, and high-performance aircraft. Teams conducted aerodynamic measurements and improved test-article access for instrumentation, enabling more precise evaluations of advanced aircraft concepts. Engineers continued developing tools and techniques to study aircraft performance under high-speed and high-temperature conditions, supporting research in hypersonic flight.

• The Sustainable Flight Demonstrator research team measured airflow over key wing surfaces in a series of wind tunnel tests, generating data used to refine future sustainable aircraft designs.
• Technicians at NASA Armstrong installed a custom structural floor inside the X-66 demonstrator, improving access for instrumentation work and enabling more efficient modification and evaluation.
• Armstrong engineers advanced high-speed research by maturing an optical measurement system that tracks heat and structural strain during hypersonic flight, supporting future test missions.

Transforming air mobility and new aviation systems

NASA Armstrong supported multiple aspects of the nation’s growing air mobility ecosystem. Researchers conducted tests and evaluations to better understand aircraft performance, airflow, and passenger experience. Additional work included assessing drone-based inspection techniques, developing advanced communication networks, performing drop tests, and refining methods to evaluate emerging mobility aircraft.

These studies support NASA’s broader goal of integrating new electric, autonomous, and hybrid aircraft safely into the national airspace.

• A small business partnership demonstrated drone-based inspection techniques that could reduce maintenance time and improve safety for commercial aircraft operations.
• NASA Armstrong researchers tested air traffic surveillance technology against the demands of air taxis flying at low altitudes through densely populated cities, using the agency’s Pilatus PC-12 to support safer air traffic operations.
• Researchers at NASA Armstrong collected airflow data from Joby using a ground array of sensors to examine how its circular wind patterns might affect electric air taxi performance in future urban operations.
• NASA Armstrong’s Ride Quality Laboratory conducted air taxi passenger comfort studies in support of the agency’s Advanced Air Mobility mission to better understand how motion, vibration, and other factors affect ride comfort, informing the industry’s development of electric air taxis and drones.

Earth observation and environmental research

Earth science campaigns at NASA Armstrong contributed to the agency’s ability to monitor environmental changes and improve satellite data accuracy. Researchers tested precision navigation systems that keep high-speed aircraft on path, supporting more accurate atmospheric and climate surveys. Airborne measurements and drone flights documented wildfire behavior, smoke transport, and post-fire impacts while gathering temperature, humidity, and airflow data during controlled burns. These efforts also supported early-stage technology demonstrations, evaluating new wildfire sensing tools under real flight conditions to advance fire response research. High-altitude aircraft contributed to missions that improved satellite calibration, refined atmospheric measurements, and supported snowpack and melt studies to enhance regional water-resource forecasting.

• Researchers at NASA Armstrong tested a new precision‑navigation system that can keep high‑speed research aircraft on exact flight paths, enabling more accurate Earth science data collection during airborne environmental and climate‑survey missions.
• NASA’s B200 King Air flew over wildfire‑affected regions equipped with the Compact Fire Infrared Radiance Spectral Tracker (c‑FIRST), collecting thermal‑infrared data to study wildfire behavior, smoke spread, and post‑fire ecological impacts in near real time.
• NASA Armstrong’s Alta X drone carried a 3D wind sensor and a radiosonde to measure temperature, pressure, humidity, and airflow during a prescribed burn in Geneva State Forest, gathering data to help improve wildland fire behavior models and support firefighting agencies.
• NASA’s ER‑2 aircraft carried the Airborne Lunar Spectral Irradiance (air-LUSI) instrument on night flights, measuring moonlight reflectance to generate calibration data – improving the accuracy of Earth‑observing satellite measurements.
• The center’s ER-2 also flew above cloud layers with specialized instrumentation to collect atmospheric and cloud measurements. These data help validate and refine Earth observing satellite retrievals, improving climate, weather, and aerosol observations.
• Airborne campaigns at NASA Armstrong measured snowpack and melt patterns in the western U.S., providing data to improve water-resource forecasting for local communities.

Exploration technology and Artemis support

NASA Armstrong supported exploration technologies that will contribute to agency’s return to the Moon and future missions deeper into the solar system, including sending the first astronauts – American astronauts – to Mars. Teams advanced sensor systems and conducted high-altitude drop tests to capture critical performance data, supporting the need for precise entry, descent, and landing capabilities on future planetary missions.

Contributions from NASA Armstrong also strengthen the systems and technologies that help make Artemis – the agency’s top priority – safer, more reliable, and more scientifically productive, supporting a sustained human presence on the Moon and preparing for future human exploration of Mars.

• The EPIC team at NASA Armstrong conducted research flights to advance sensor technology for supersonic parachute deployments, evaluating performance during high-speed, high-altitude drops relevant to future planetary missions.
• Imagery from the EPIC test flights at NASA Armstrong highlights the parachute system’s high-altitude deployment sequence and demonstrated its potential for future Mars delivery concepts.

People, workforce, and community engagement

The center expanded outreach, education, and workforce development efforts throughout the year. Students visited NASA Armstrong for hands-on exposure to careers in aeronautics, while staff and volunteers supported a regional robotics competition that encouraged exploration of the field. Educators brought aeronautics concepts directly into classrooms across the region, and interns from around the country gained experience supporting real flight research projects.

NASA Armstrong also highlighted unique career pathways and recognized employees whose work showcases the human side of NASA missions. A youth aviation program launched with a regional museum provided additional opportunities for young learners to explore flight science, further strengthening the center’s community impact:

• Students from Palmdale High School Engineering Club visited NASA Armstrong, where staff engaged with them to explore facilities, discuss aerospace work, and promote STEM careers as part of the center’s community outreach.
• NASA Armstrong staff and volunteers mentored high school teams at the 2025 Aerospace Valley FIRST Robotics Competition, helping students build and test robots and providing hands-on experience with engineering to foster interest in STEM careers.
• In April, NASA Armstrong expanded outreach in 2025 by bringing aeronautics concepts to students through classroom workshops, presentations, and hands-on activities, giving young learners direct exposure to NASA research and inspiring possible future careers in science and engineering.
• Students from across the country participated in internships at NASA Armstrong, gaining hands-on experience in flight research and operations while contributing to real-world aerospace projects.
• In May, a NASA Armstrong videographer earned national recognition for work that highlights the people behind the center’s research missions, showing how scientists, engineers, and flight crews collaborate to advance aeronautics and space exploration.
• Daniel Eng, a systems engineer with NASA’s Air Mobility Pathfinders project, shared his career path from the garment industry to aerospace, illustrating how diverse experiences contribute to the center’s technical workforce and support its advanced flight research and engineering projects.
• In June, NASA Armstrong recognized one of its interns for hands-on work with the center’s aircraft. With more than a decade in the auto industry, they demonstrated how early career engineers can gain real-world experience and develop skills for careers in aerospace and flight research.
• NASA Armstrong partnered with a regional museum to create a youth aviation program that introduces students to flight science and operations, providing hands-on learning opportunities and inspiring interest in aerospace and STEM careers.

Center infrastructure and research capabilities

Facility improvements and new platforms strengthened NASA Armstrong’s research capabilities. A rooftop operation removed a historic telemetry pedestal to make way for updated infrastructure, while preserving an important artifact of the center’s flight test heritage. Engineers also completed a new subscale research aircraft, providing a flexible, cost-effective platform for evaluating aerodynamics, instrumentation, and flight control concepts in preparation for full-scale testing:

• The center improved workspace access and supported a re-roofing project during a helicopter crew operation that removed a 2,500-pound telemetry pedestal from a building rooftop, preserving a piece of the center’s flight history heritage.
• Engineers at NASA Armstrong built a new subscale experimental aircraft to replace the center’s aging MicroCub. The 14-foot wingspan, 60-pound aircraft provides a flexible, cost-effective platform for testing aerodynamics, instrumentation, and flight control concepts while reducing risk before full-scale or crewed flight tests.

Looking ahead

NASA Armstrong will continue advancing flight research across aeronautics and Earth science, building on this year’s achievements. Upcoming efforts include additional X-59 flights, expanded quiet supersonic studies, new air mobility evaluations, high-altitude science campaigns, and maturing technologies that support hypersonic research and the Artemis program for future planetary missions.

“Next year will be a year of continuity, but also change,” Flick said. “The agency’s new Administrator, Jared Isaacman, will bring a renewed mission-first focus to the agency, and NASA Armstrong will push the boundaries of what’s possible. But the most important thing we can do is safely and successfully execute our portfolio of work within budget and schedule.”

For more than seven decades, NASA Armstrong has strengthened the nation’s understanding of flight. This year’s work builds on that legacy, helping shape the future of aviation and exploration through research proven in the air.

To explore more about NASA Armstrong’s missions, research, and discoveries, visit:

https://www.nasa.gov/armstrong

The four astronauts set to fly around the Moon during NASA’s Artemis II test flight depart the Neil A. Armstrong Operations and Checkout Building at the agency’s Kennedy Space Center in Florida, during a dress rehearsal for launch day on Dec. 20, 2025. From left are CSA (Canadian Space Agency) astronaut Jeremy Hansen, NASA astronauts Victor Glover, Reid Wiseman, and Christina Koch.

The launch day rehearsal, called a countdown demonstration test, simulated the launch day timeline, including the crew suiting up in their spacesuits and climbing in and out of their Orion spacecraft. Because the SLS (Space Launch System) rocket upon which they will launch is not yet at the launch pad, the crew boarded Orion inside Kennedy’s Vehicle Assembly Building, where engineers are conducting final preparations on the spacecraft, rocket, and ground systems.  

Through Artemis, NASA will send astronauts to explore the Moon for scientific discovery, economic benefits, and build the foundation for the first crewed missions to Mars.

Photo Credit: NASA/Jim Ross

Written by Noah Martin, Ph.D. student and Candice Bedford, Research Scientist at Purdue University

While much of Perseverance’s work focuses on ancient rocks that record Mars’ long-lost rivers and lakes, megaripples offer a rare opportunity to examine processes that are still shaping the surface today. Megaripples are sand ripples up to 2 meters (about 6.5 feet) tall that are mainly built and modified by wind. However, when water in the atmosphere interacts with dust on the ripple surface, a salty, dusty crust can form. When this happens, it is much harder for the wind to move or shape the megaripple. As such, megaripples on Mars are largely considered inactive, standing as records of past wind regimes and atmospheric water interactions over time. However, some have shown signs of movement, and it is possible that periods of high wind speeds may erode or reactivate these deposits again.

Despite Mars’ thin atmosphere today (2% of the Earth’s atmospheric density), wind is one of the main drivers of change at the surface, eroding local bedrock into sand-sized grains and transporting these grains across the ripple field. As a result, megaripple studies help us understand how wind has shaped the surface in Mars’ most recent history and support planning for future human missions, as the chemistry and cohesion of Martian soils will influence everything from mobility to resource extraction.

Following the successful investigation of the dusty, inactive megaripples at “Kerrlaguna,” Perseverance recently explored a more expansive field of megaripples called “Honeyguide.” This region hosts some of the largest megaripples Perseverance has seen along its traverse so far, making it an ideal location for a comprehensive study of these features. The megaripples at “Honeyguide” rise higher, extend farther, and have sharply defined crests with more uniform orientation compared to those at “Kerrlaguna.” The consistent orientation of the megaripples at “Honeyguide” suggests that winds in this area have blown predominantly from the same direction (north-south) for a long period of time.

At “Honeyguide,” Perseverance studied the “Hazyview” megaripple, where over 50 observations were taken across the SuperCam, Mastcam-Z, MEDA, PIXL and WATSON instruments, looking for grain movement, signs of early morning frost, and changes in mineralogy from crest to trough. The investigation of the “Hazyview” bedform builds directly on the results from “Kerrlaguna” and represents the most detailed look yet at these intriguing wind-formed deposits. As Perseverance continues its journey on the crater rim, these observations will provide a valuable reference for interpreting other wind-blown features and for understanding how Mars continues to change, one grain of sand at a time.

As part of NASA’s SpaceX Crew-12 mission, four crew members from three space agencies will launch no earlier than Sunday, Feb. 15, 2026, to the International Space Station for a long-duration science expedition.

NASA astronauts Jessica Meir and Jack Hathaway will serve as spacecraft commander and pilot, respectively, and will be accompanied by ESA (European Space Agency) astronaut Sophie Adenot and Roscosmos cosmonaut Andrey Fedyaev, who will both serve as mission specialists. Crew-12 will join Expedition 74 crew members currently aboard the space station.

The flight is the 12th crew rotation with SpaceX to the orbiting laboratory as part of NASA’s Commercial Crew Program. Crew-12 will conduct scientific investigations and technology demonstrations to help prepare humans for future exploration missions to the Moon and Mars, as well as benefit people on Earth.

This will be the second flight to the space station for Meir, who was selected as a NASA astronaut in 2013. The Caribou, Maine, native earned a bachelor’s degree in biology from Brown University, a master’s degree in space studies from the International Space University, and a doctorate in marine biology from Scripps Institution of Oceanography in San Diego. On her first spaceflight, Meir spent 205 days as a flight engineer during Expedition 61/62, and she completed the first three all-woman spacewalks with fellow NASA astronaut Christina Koch, totaling 21 hours and 44 minutes outside of the station. Since then, she has served in various roles, including assistant to the chief astronaut for commercial crew (SpaceX), deputy for the Flight Integration Division, and assistant to the chief astronaut for the human landing system.

A commander in the United States Navy, Hathaway was selected as part of the 2021 astronaut candidate class. This will be Hathaway’s first spaceflight. The South Windsor, Connecticut, native holds a bachelor’s degree in physics and history from the U.S. Naval Academy and master’s degrees in flight dynamics from Cranfield University and national security and strategic studies from the U.S. Naval War College, respectively. Hathaway also is a graduate of the Empire Test Pilot’s School, Fixed Wing Class 70 in 2011. At the time of his selection, Hathaway was deployed aboard the USS Truman, serving as Strike Fighter Squadron 81’s prospective executive officer. He has accumulated more than 2,500 flight hours in 30 different aircraft, including more than 500 carrier arrested landings and 39 combat missions.

The Crew-12 mission will be Adenot’s first spaceflight. Before her selection as an ESA astronaut in 2022, Adenot earned a degree in engineering from ISAE-SUPAERO in Toulouse, France, specializing in spacecraft and aircraft flight dynamics. She also earned a master’s degree in human factors engineering at Massachusetts Institute of Technology in Cambridge. After earning her master’s degree, she became a helicopter cockpit design engineer at Airbus Helicopters and later served as a search and rescue pilot at Cazaux Air Base from 2008 to 2012. She then joined the High Authority Transport Squadron in Villacoublay, France, and served as a formation flight leader and mission captain from 2012 to 2017. Between 2019 and 2022, Adenot worked as a helicopter experimental test pilot in Cazaux Flight Test Center with DGA (Direction Générale de l’Armement – the French Defence Procurement Agency). She has logged more than 3,000 hours flying 22 different helicopters.

This will be Fedyaev’s second long-duration stay aboard the orbiting laboratory. He graduated from the Krasnodar Military Aviation Institute in 2004, specializing in aircraft operations and air traffic organization, and earned qualifications as a pilot engineer. Prior to his selection as a cosmonaut, he served as deputy commander of an Ilyushin-38 aircraft unit in the Kamchatka Region, logging more than 600 flight hours and achieving the rank of second-class military pilot. Fedyaev was selected for the Gagarin Research and Test Cosmonaut Training Center Cosmonaut Corps in 2012 and has served as a test cosmonaut since 2014. In 2023, he flew to the space station as a mission specialist during NASA’s SpaceX Crew-6 mission, spending 186 days in orbit, as an Expedition 69 flight engineer. For his achievements, Fedyaev was awarded the title Hero of the Russian Federation and received the Yuri Gagarin Medal. 

For more than 25 years, people have lived and worked continuously aboard the International Space Station, advancing scientific knowledge and making research breakthroughs that are not possible on Earth. The station is a critical testbed for NASA to understand and overcome the challenges of long-duration spaceflight and to expand commercial opportunities in low Earth orbit. As commercial companies concentrate on providing human space transportation services and destinations as part of a robust low Earth orbit economy, NASA is focusing its resources on deep space missions to the Moon as part of the Artemis campaign in preparation for future human missions to Mars.

Learn more about International Space Station research and operations at:

https://www.nasa.gov/station

-end-

Joshua Finch / Jimi Russell
Headquarters, Washington
202-358-1100
joshua.a.finch@nasa.gov / james.j.russell@nasa.gov

Shaneequa Vereen
Johnson Space Center, Houston
281-483-5111
shaneequa.y.vereen@nasa.gov

NASA’s Johnson Space Center in Houston closed 2025 with major progress across human spaceflight, research, and exploration. From Artemis II mission preparations to science aboard the International Space Station, teams at Johnson helped prepare for future missions to the Moon and, ultimately, Mars.

Orion Stacked for Artemis II, Orion Mission Evaluation Room Unveiled 

As NASA prepares for the crewed Artemis II mission, a 10-day journey around the Moon and back in early 2026, teams at Johnson continue work to ensure the Orion spacecraft is flight-ready. The mission will carry NASA astronauts Reid Wiseman, Victor Glover, Christina Koch, and CSA (Canadian Space Agency) astronaut Jeremy Hansen. 

In October, NASA completed stacking of the Orion spacecraft and launch abort system atop the agency’s SLS (Space Launch System) rocket inside the Vehicle Assembly Building at NASA’s Kennedy Space Center in Florida. Following Orion stacking, teams completed testing critical communications systems between SLS and Orion, and confirmed the interfaces function properly between the rocket, Orion, and the ground systems. 

Teams also unveiled the Orion Mission Evaluation Room inside NASA’s Mission Control Center in Houston. The new facility will support Artemis II by allowing engineers to monitor Orion spacecraft systems in real time and assess vehicle performance throughout the mission, strengthening flight operations beyond low Earth orbit. 

These milestones were made possible by teams across Johnson, including the Orion Program, Flight Operations Directorate, Systems Engineering and Integration Office, Crew and Thermal Systems Division, and the Human Health and Performance Directorate, working closely with other NASA centers and industry partners. 

Together, these accomplishments mark steady progress toward Artemis II and reflect the work underway across NASA to advance the next era of human spaceflight. 

Gateway Lunar Space Station

Together with international and industry partners, the Gateway Program continued progress toward building humanity’s first lunar space station. The powerhouse reached a major milestone this fall with its successful initial power on.

A Space Station Anniversary

On Nov. 2, 2025, NASA marked 25 years of continuous human presence aboard the space station. What began as a set of connected modules has grown into a cornerstone of international partnership, scientific discovery, and technology development in low Earth orbit.
For a quarter of century, the orbiting laboratory has supported research that advances human health, drives innovation, and prepares NASA for future crewed missions to the Moon and Mars.

A truly global endeavor, the space station has been visited by more than 290 people from 26 countries and a variety of international and commercial spacecraft. The unique microgravity laboratory has hosted more than 4,000 experiments from over 5,000 researchers from 110 countries. The orbital outpost also is facilitating the growth of a commercial market in low Earth orbit for research, technology development, and crew and cargo transportation.

After 25 years of habitation, the space station remains a symbol of international cooperation and a proving ground for humanity’s next giant leaps.

Record-Breaking Spacewalks

NASA astronauts Nick Hague, Suni Williams, and Butch Wilmore began 2025 with two successful spacewalks, completing key maintenance and research tasks. Their work included removing an antenna assembly and collecting surface material samples for analysis at Johnson’s Astromaterials Research and Exploration Services, or ARES, division.

With her latest spacewalks, Williams now holds the record for the most cumulative spacewalking time by a woman–62 hours and 6 minutes–placing her fourth among the most experienced spacewalkers.

NASA astronauts Anne McClain and Nichole Ayers also conducted spacewalk operations, installing a mounting bracket to prepare for the future installation of an additional set of International Space Station Rollout Solar Arrays and relocating a space station communications antenna.

These achievements were made possible by countless Johnson teams across the International Space Station, Flight Operations Directorate, and Exploration Architecture, Integration, and Science Directorate.

Two Expeditions Take Flight

NASA’s SpaceX Crew-10 arrived at the space station on March 15 and returned to Earth on on Aug. 9. Crew-10 included NASA astronauts Anne McClain and Nichole Ayers, JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi, and Roscosmos cosmonaut Kirill Peskov—all of whom are trained pilots. Crew-9 also splashed down off Florida’s coast on March 18. 

NASA astronaut Jonny Kim launched aboard the Soyuz MS-27 spacecraft on April 8, marking his first mission to the space station. Expedition 73 officially began following the departure of NASA astronaut Don Pettit aboard Soyuz MS-26 on April 19. NASA astronaut Chris Williams then launched aboard the Soyuz MS-28 spacecraft on Nov. 27 with Kim returning to Earth shortly after on Dec. 9, marking the start of Expedition 74.

NASA Selects 2025 Astronaut Candidate Class

NASA’s 10 new astronaut candidates were introduced Sept. 22 following a competitive selection process of more than 8,000 applicants from across the United States. The class will complete nearly two years of training before becoming eligible for flight assignments supporting missions to low Earth orbit, the Moon, and Mars.

When they graduate, they will join NASA’s active astronaut corps, advancing research aboard the space station and supporting Artemis missions that will carry human exploration farther than ever before.

A Year of Lunar Firsts

Firefly Aerospace’s Blue Ghost Mission 1 launched delivering 10 NASA science and technology instruments to the Moon on March 2. The lander touched down near Mons Latreille in Mare Crisium, a basin on the near side of the Moon. Just days later on March 6, Intuitive Machines’ IM-2 mission landed closer to the lunar South Pole than any previous lander.  

Part of NASA’s Commercial Lunar Payload Services (CLPS) and Artemis campaign, these lunar deliveries are helping scientists address challenges like lunar dust mitigation, resource utilization, and radiation tolerance. 

These milestones were made possible by the collaborative efforts of Johnson teams across NASA’s CLPS initiative, as well as the Engineering; Exploration Architecture, Integration, and Science; and Flight Operations directorates—along with support from other NASA centers. 

First Asteroid-Detecting Space Telescope Completes Testing

NASA’s Near-Earth Object (NEO) Surveyor—its first space-based telescope designed specifically for planetary defense—has successfully completed thermal vacuum testing in Johnson’s Space Environment Simulation Laboratory in Chamber A. 

Set to launch no earlier than late 2027, NEO Surveyor will seek out, measure, and characterize hard-to-detect asteroids and comets that could pose a hazard to Earth. The spacecraft is now at NASA’s Jet Propulsion Laboratory in Southern California for continued development. 

Explore the capabilities and scientific work enabled by the thermal testing conducted in Johnson’s Chamber A. 

These achievements were made possible by countless Johnson teams across the ARES Division and Engineering Directorate. 

First Houston AutoBoative Show

For the first time, NASA rolled out its Artemis exhibit at the Houston AutoBoative Show at NRG Center from Jan. 29 to Feb. 2. Johnson employees introduced vehicle enthusiasts to the technologies NASA and its commercial partners will use to explore more of the lunar surface than ever before.

The Artemis exhibit stood alongside some of the world’s most advanced cars and boats, offering visitors an up-close look at the future of human space exploration.

Attendees explored Artemis II and Artemis III mission road maps, practiced a simulated Orion docking with Gateway in lunar orbit, and tested their skills driving a virtual lunar rover simulator.

NASA showcased lunar rover concepts, highlighting vehicles under development to help Artemis astronauts travel farther across the Moon’s surface.

All three Lunar Terrain Vehicle (LTV) contractors, Astrolab, Intuitive Machines, and Lunar Outpost, completed their Preliminary Design Review milestones in June 2025, marking the end of Phase 1 feasibility study task orders that began in May 2024. NASA is preparing to award Phase 2 of the Lunar Terrain Vehicle Services contract with a demonstration mission task order that will result in the development, delivery, and demonstration of an LTV on the Moon  later this decade.

First Dual NBL Run for NASA’s Artemis III Lunar Spacesuit

NASA and Axiom Space teams held the first dual spacesuit run at NASA’s Neutral Buoyancy Laboratory with NASA astronauts Stan Love and Loral O’Hara. Both crewmembers wore Axiom Space’s lunar spacesuit, called the Axiom Extravehicular Mobility Unit (AxEMU), while performing simulated lunar surface operations underwater to test the spacesuit’s functionality and mobility. This was the final integration test in the pool, proving both the spacesuit and facility are ready to support NASA Artemis training. To date, the Axiom team has conducted over 700 hours of manned, pressurized testing of the Artemis III lunar spacesuit. Axiom Space is scheduled to complete the critical design review in 2026.

These efforts were made possible by teams across Johnson’s Joint Extravehicular Activity and Human Surface Mobility Test Team.

Watch how astronauts, engineers, and scientists are preparing for the next giant leap on the lunar surface.

OSIRIS-REx Team Honored for Asteroid Sample Return

NASA’s OSIRIS-REx curation team earned an Agency Group Achievement Award for their dedication to acquiring, preserving, and distributing asteroid samples from Bennu—the agency’s first asteroid sample return mission.

“The curation team ensured we were ready to receive and safeguard the samples, prepare and allocate them, and make them available to the broader scientific community,” said Jemma Davidson, Astromaterials curator and branch chief of the Astromaterials Acquisition and Curation Office.

After years of preparation, the team overcame unforeseen technical challenges to recover and preserve more than 120 grams of asteroid material—now accessible to scientists worldwide for research into the origins of our solar system.

These achievements were made possible by Johnson teams across the ARES Division and the Exploration Architecture, Integration, and Science Directorate.

Axiom Mission 4 Marks International Firsts in Space Station Mission 

The Axiom Mission 4 crew successfully returned to Earth after an 18-day mission aboard the space station, conducting more than 60 experiments and educational outreach activities. Launched aboard a SpaceX Dragon spacecraft on June 25, the crew docked with the orbiting laboratory the following day to begin a packed schedule of science and outreach. 

The mission marked the first space station flight for India, Poland, and Hungary. Led by former NASA astronaut and Axiom Space director of human spaceflight Peggy Whitson, the crew included ISRO (Indian Space Research Organization) astronaut Shubhanshu Shukla, ESA (European Space Agency) project astronaut Sławosz Uznański-Wiśniewski of Poland, and Hungarian to Orbit (HUNOR) astronaut Tibor Kapu. 

These achievements were made possible by Johnson’s dedicated teams across the International Space Station Program, Commercial Low Earth Orbit Development Program, and Flight Operations Directorate. 

Johnson-Built Mars Hardware on Display at the Smithsonian 

A piece of NASA Johnson Space Center’s Mars legacy has landed at the Smithsonian National Air and Space Museum in Washington, D.C. 

Nearly 10 years in the making, the Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals (SHERLOC) calibration target—built by Johnson’s ARES Division with partners at NASA’s Jet Propulsion Laboratory and Amentum—now has a permanent place in the museum’s Futures in Space gallery.  

The palm-sized device is displayed beside an R2-D2 replica, connecting the wonder of space travel with the inspiration of seeing real flight hardware up close. 

The calibration target, still in use aboard NASA’s Perseverance rover after more than four years of operations in Jezero Crater, Mars, helps keep SHERLOC’s laser, cameras, and spectrometers precisely tuned as it searches for ancient signs of life on Mars. Mounted on the rover’s front, the target carries 10 known samples so engineers can check SHERLOC’s performance during routine operations. 

Trevor Graff, an ARES scientist who conceived the idea and led the team that designed and built SHERLOC’s calibration device, said the project highlights the unique role of geology in space exploration. “What excites me most is the practical application of geology—where science enables exploration and exploration enables science,” he said.  

SHERLOC itself sits on the rover’s seven-foot robotic arm and combines a laser, camera, and chemical analyzers to look for signs that water once altered the Martian surface, potentially revealing evidence of past microscopic life. Several calibration targets are made from spacesuit material samples, allowing Johnson scientists to study how fabrics endure the harsh Martian environment to protect future explorers. 

Just like your cellphone stays connected by roaming between networks, NASA’s Polylingual Experimental Terminal, or PExT, technology demonstration is proving space missions can do the same by switching seamlessly between government and commercial communications networks.

NASA missions rely on critical data to navigate, monitor spacecraft health, and transmit scientific information back to Earth, and this game-changing technology could provide multiple benefits to government and commercial missions by enabling more reliable communications with fewer data interruptions.

“This mission has reshaped what’s possible for NASA and the U.S. satellite communications industry,” said Kevin Coggins, deputy associate administrator for the agency’s SCaN (Space Communications and Navigation) Program at NASA Headquarters in Washington. “PExT demonstrated that interoperability between government and commercial networks is possible near-Earth, and we’re not stopping there. The success of our commercial space partnerships is clear, and we’ll continue to carry that momentum forward as we expand these capabilities to the Moon and Mars.”

Wideband technology enables data exchange across a broad range of frequencies, helping bridge government and commercial networks as NASA advances commercialization of space communications. By providing interoperability between government and commercial assets, this technology unlocks new advantages not currently available to agency missions.

As commercial providers continue to advance their technology and add new capabilities to their networks, missions equipped with wideband terminals can integrate these enhancements even after launch and during active operations. The technology also supports NASA’s network integrity by allowing missions to seamlessly switch back and forth between providers if one network faces critical disruptions that would otherwise interfere with timely communications.

“Today, we take seamless cellphone roaming for granted, but in the early days of mobile phones, our devices only worked on one network,” said Greg Heckler, SCaN’s capability development lead at NASA Headquarters. “Our spaceflight missions faced similar limitations—until now. These revolutionary tests prove wideband terminals can connect spacecraft to multiple networks, a huge benefit for early adopter missions transitioning to commercial services in the 2030s.”

On July 23, the communications demo launched into low Earth orbit aboard the York Space Systems’ BARD mission. Designed by Johns Hopkins Applied Physics Laboratory, the compact wideband terminal communicates over a broad range of the Ka-band frequency, which is commonly used by NASA missions and commercial providers. After completing a series of tests that proved the BARD spacecraft and the demonstration payload were functioning as expected, testing kicked off with NASA’s TDRS (Tracking and Data Relay Satellite) fleet and commercial satellite networks operated by SES Space & Defense and Viasat.

During each demonstration, the terminal completed critical space communications and navigation operations, ranging from real-time spacecraft tracking and mission commands to high-rate data delivery. By showcasing end-to-end services between the BARD spacecraft, multiple commercial satellites, and mission control on Earth, the wideband terminal showed future NASA missions could become interoperable with government and commercial infrastructure.

Due to the flexibility of wideband technology and the innovative nature of this mission, NASA recently extended the Polylingual Experiment Terminal demonstration for an additional 12 months of testing. Extended mission operations will include new direct-to-Earth tests with the Swedish Space Corporation, scheduled to begin in early 2026.

This technology demonstration will continue testing spaceflight communications capabilities through April 2027. By 2031, NASA plans to purchase satellite relay services for science missions in low Earth orbit from one or more U.S. companies.

To learn more about this wideband technology demonstration visit:

PExT – NASA

The Polylingual Experimental Terminal technology demonstration is funded and managed by NASA’s SCaN Program within the Space Operations Mission Directorate at NASA Headquarters in Washington. York Space Systems provided the host spacecraft. Johns Hopkins Applied Physics Laboratory developed the demonstration payload. Commercial satellite relay demonstrations were conducted in partnership with SES Space & Defense and Viasat.

NASA astronaut Don Pettit demonstrates electrostatic forces using charged water droplets and a knitting needle made of Teflon. This series of overlapping frames from Feb. 19, 2025, displays the unique attraction-repulsion properties of Teflon and charged droplets, similar to how charged particles from the Sun behave when they come in contact with Earth’s magnetic field. Highly energetic particles from space that collide with atoms and molecules in the atmosphere create the aurora borealis.

Explore more of what Pettit has coined “science of opportunity.”

Image credit: NASA/Don Pettit