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Perseverance Rover Witnesses One Martian Dust Devil Eating Another
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Preparations for Next Moonwalk Simulations Underway (and Underwater) A Martian dust devil can be seen consuming its smaller friend in this short video made of images taken at the rim of Jezero Crater by NASA’s Perseverance Mars rover on Jan. 25, 2025. NASA/JPL-Caltech/SSIThe six-wheeled explorer recently captured several Red Planet mini-twisters spinning on the rim of Jezero Crater.
A Martian dust devil can be seen consuming a smaller one in this short video made of images taken by a navigation camera aboard NASA’s Perseverance Mars rover. These swirling, sometimes towering columns of air and dust are common on Mars. The smaller dust devil’s demise was captured during an imaging experiment conducted by Perseverance’s science team to better understand the forces at play in the Martian atmosphere.
When the rover snapped these images from about 0.6 miles (1 kilometer) away, the larger dust devil was approximately 210 feet (65 meters) wide, while the smaller, trailing dust devil was roughly 16 feet (5 meters) wide. Two other dust devils can also be seen in the background at left and center. Perseverance recorded the scene Jan. 25 as it explored the western rim of Mars’ Jezero Crater at a location called “Witch Hazel Hill.”
“Convective vortices — aka dust devils — can be rather fiendish,” said Mark Lemmon, a Perseverance scientist at the Space Science Institute in Boulder, Colorado. “These mini-twisters wander the surface of Mars, picking up dust as they go and lowering the visibility in their immediate area. If two dust devils happen upon each other, they can either obliterate one another or merge, with the stronger one consuming the weaker.”
While exploring the rim of Jezero Crater on Mars, NASA’s Perseverance rover captured new images of multiple dust devils in January 2025. These captivating phenomena have been documented for decades by the agency’s Red Planet robotic explorers. NASA/JPL-Caltech/LANL/CNES/CNRS/INTA-CSIC/Space Science Institute/ISAE-Supaero/University of Arizona Science of WhirlwindsDust devils are formed by rising and rotating columns of warm air. Air near the planet’s surface becomes heated by contact with the warmer ground and rises through the denser, cooler air above. As other air moves along the surface to take the place of the rising warmer air, it begins to rotate. When the incoming air rises into the column, it picks up speed like a spinning ice skater bringing their arms closer to their body. The air rushing in also picks up dust, and a dust devil is born.
“Dust devils play a significant role in Martian weather patterns,” said Katie Stack Morgan, project scientist for the Perseverance rover at NASA’s Jet Propulsion Laboratory in Southern California. “Dust devil study is important because these phenomena indicate atmospheric conditions, such as prevailing wind directions and speed, and are responsible for about half the dust in the Martian atmosphere.”
NASA’s Viking 1 orbiter captured this Martian dust devil casting a shadow on Aug. 1, 1978. During the 15-second interval between the two images, the dust devil moved toward the northeast (toward the upper right) at a rate of about 59 feet (18 meters) per second. NASA/JPL-Caltech/MSSSSince landing in 2021, Perseverance has imaged whirlwinds on many occasions, including one on Sept. 27, 2021, where a swarm of dust devils danced across the floor of Jezero Crater and the rover used its SuperCam microphone to record the first sounds of a Martian dust devil.
NASA’s Viking orbiters, in the 1970s, were the first spacecraft to photograph Martian dust devils. Two decades later, the agency’s Pathfinder mission was the first to image one from the surface and even detected a dust devil passing over the lander. Twin rovers Spirit and Opportunity managed to capture their fair share of dusty whirlwinds. Curiosity, which is exploring a location called Mount Sharp in Gale Crater on the opposite side of the Red Planet as Perseverance, sees them as well.
Capturing a dust devil image or video with a spacecraft takes some luck. Scientists can’t predict when they’ll appear, so Perseverance routinely monitors in all directions for them. When scientists see them occur more frequently at a specific time of day or approach from a certain direction, they use that information to focus their monitoring to try to catch additional whirlwinds.
“If you feel bad for the little devil in our latest video, it may give you some solace to know the larger perpetrator most likely met its own end a few minutes later,” said Lemmon. “Dust devils on Mars only last about 10 minutes.”
More About PerseveranceA key objective of Perseverance’s mission on Mars is astrobiology, including caching samples that may contain signs of ancient microbial life. The rover is characterizing the planet’s geology and past climate, to help pave the way for human exploration of the Red Planet and as the first mission to collect and cache Martian rock and regolith.
NASA’s Mars Sample Return Program, in cooperation with ESA (European Space Agency), is designed to send spacecraft to Mars to collect these sealed samples from the surface and return them to Earth for in-depth analysis.
The Mars 2020 Perseverance mission is part of NASA’s Mars Exploration Program (MEP) portfolio and the agency’s Moon to Mars exploration approach, which includes Artemis missions to the Moon that will help prepare for human exploration of the Red Planet.
NASA’s Jet Propulsion Laboratory, which is managed for the agency by Caltech, built and manages operations of the Perseverance rover.
For more about Perseverance:
https://science.nasa.gov/mission/mars-2020-perseverance
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La NASA aumenta su eficiencia con un piso modificado para el avión X-66
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Eric Garza, técnico de ingeniería en el Taller de Fabricación Experimental del Centro de Investigación de Vuelos Armstrong de la NASA en Edwards, California, corta madera contrachapada a medida para las tablas del piso temporal del avión demostrador experimental X-66 el 26 de agosto de 2024.NASA/Steve FreemanRead this story in English here.
La NASA diseño unas tablas de piso temporales para el avión MD-90, que se utilizaran mientras el avión se transforma en el demostrador experimental X-66. Estas tablas de piso protegerán el piso original y agilizarán el proceso de modificación.
En apoyo al proyecto Demostrador de Vuelo Sostenible de la agencia, un pequeño equipo del Taller de Fabricación Experimental del Centro de Investigación de Vuelos Armstrong de la NASA en Edwards, California, construyó tablas de piso temporales para ahorrarle tiempo y recursos al proyecto. La retirada e instalación repetidas del piso original durante el proceso de modificación requería mucho tiempo. El uso de paneles temporales también garantiza la protección de las tablas del piso original y su aptitud para el vuelo cuando se finalicen las modificaciones y se vuelva a instalar el piso original.
“La tarea de crear las tablas de piso temporales para el MD-90 implica un proceso meticuloso dirigido a facilitar las modificaciones, manteniendo la seguridad y la eficacia. La necesidad de estas tablas de piso temporales surge del detallado procedimiento necesario para retirar y reinstalar los pisos originales del fabricante (OEM, por su acrónimo inglés),” explica Jason Nelson, jefe de fabricación experimental. Él es uno de los dos miembros del equipo de fabricación – un técnico de ingeniería y un inspector – que fabrica acerca de 50 tablas de piso temporales, con dimensiones que varían entre 20 pulgadas por 36 pulgadas y 42 pulgadas por 75 pulgadas.
Una máquina de madera corta agujeros precisos en madera contrachapada para las tablas del piso temporal el 26 de agosto de 2024, en el Taller de Fabricación Experimental del Centro de Investigación de Vuelo Armstrong de la NASA en Edwards, California. El piso fue diseñado para el avión de demonstración experimental X-66. NASA/Steve FreemanNelson continuó, “Como estas tablas OEM se quitarán y volverán a instalar varias veces para acomodar las modificaciones necesarias, las tablas temporales ahorrarán al equipo tiempo y recursos valiosos. También proporcionarán el mismo nivel de seguridad y resistencia que las tablas OEM, garantizando que el proceso se desarrolle sin problemas y sin comprometer la calidad.”
El diseño y la creación de prototipos del piso fue un proceso meticuloso, pero la solución temporal desempeña un papel crucial en la optimización del tiempo y los recursos en los esfuerzos de la NASA por avanzar en la seguridad y la eficiencia de los viajes aéreos. El proyecto Demostrador de Vuelo Sostenible de la agencia busca informar la próxima generación de aviones pasajeros de un solo pasillo, que son las aeronaves más comunes de aviación comercial de todo el mundo. La NASA se asoció con Boeing para desarrollar el avión de demostración experimental X-66. El Taller de Fabricación Experimental de Armstrong de la NASA lleva a cabo modificaciones y trabajos de reparación en aeronaves, que van desde la creación de algo tan pequeño como un soporte de aluminio hasta la modificación de la estructura principal de las alas, las costillas del fuselaje, las superficies de control y otras tareas de apoyo a las misiones.
Eric Garza, técnico de ingeniería en el Taller de Fabricación Experimental del Centro de Investigación de Vuelo Armstrong de la NASA en Edwards, California, observa cómo una máquina de madera corta agujeros para las tablas del piso temporal el 26 de agosto de 2024. El piso fue diseñado para el avión de demostración experimental X-66. NASA/Steve FreemanArtículo Traducido por: Priscila Valdez
Share Details Last Updated Apr 03, 2025 EditorDede DiniusContactSarah Mannsarah.mann@nasa.gov Related Terms Explore More 4 min read El X-59 de la NASA completa las pruebas electromagnéticas Article 3 weeks ago 11 min read La NASA identifica causa de pérdida de material del escudo térmico de Orion de Artemis I Article 4 months ago 10 min read Preguntas frecuentes: La verdadera historia del cuidado de la salud de los astronautas en el espacio Article 4 months ago Keep Exploring Discover More Topics From NASAArmstrong Flight Research Center
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NASA Langley’s Legacy of Landing
Landing safely on the surface of another planetary body, like the Moon or Mars, is one of the most important milestones of any given space mission. From the very beginning, NASA’s Langley Research Center has been at the heart of the entry, descent and landing (EDL) research that enables our exploration. Today, NASA Langley’s legacy of landing continues at the forefront of present day lunar missions and as NASA prepares for future travel to more distant worlds.
Project Mercury: 1958Project Mercury was the United States’ first human-in-space program, led by NASA’s Space Task Group located at NASA Langley. There were five major programs of study and experimentation.
- An airdrop study that helped us understand the characteristics of the Mercury capsule as it returned to Earth.
- A group of study focused on the escape systems, ultimately becoming known as the launch abort system.
- Exhaustive wind-tunnel studies of the blunt-nosed capsule design and its aerodynamic stability at various altitudes and speeds and angles of reentry, all with a focus on making the capsule safe and stable.
- A study on the problem of landing impact, resulting in the development of absorption systems that minimized the shock of impact to the capsule’s pilot.
- Studies into the use of drogue parachutes and their characteristics at high altitudes and speeds, ensuring that they would be able to stabilize and slow the capsule’s descent for a safe landing. All of this research went on to inform the subsequent Gemini and Apollo programs.
All of this research went on to inform the subsequent Gemini and Apollo programs.
Apollo Program: 1962In 1961, President John F. Kennedy committed to putting Americans on the surface of the Moon and shortly after that historic declaration, NASA’s Apollo program was born. In the years that followed, the original team of NASA astronauts completed their basic training at NASA Langley’s Lunar Landing Research Facility (LLRF). When Apollo 11 successfully landed the first humans on the Moon in 1969, NASA Langley had played a pivotal role in the monumental success.
Lunar Orbiter: 1966The Lunar Orbiter missions launched with the purpose of mapping the lunar surface and identifying potential landing sites ahead of the Apollo landings. From 1966 to 1967, the five successful Lunar Orbiter missions, led and managed by Langley Research Center, resulted in 99% of the moon photographed and a suitable site selected for the upcoming human landings.
Viking: 1976After the success of Apollo, NASA set its sights further across the solar system to Mars. Two Viking missions aimed to successfully place landers on the Red Planet and capture high resolution images of the Martian surfaces, assisting in the search for life. Langley Research Center was chosen to lead this inaugural Mars mission and went on to play key roles in the missions to Mars that followed.
HIAD: 2009 – PresentSuccessful landings on Mars led to more ambitious dreams of landing larger payloads, including those that could support future human exploration. In order to land those payloads safely, a new style of heat shield would be needed. Hypersonic Inflatable Aerodynamic Decelerator (HIAD) technology was positioned as an answer to the payload problem, enabling missions to use inflatable heat shields to slow down and protect a payload as it enters a planet’s atmosphere at hypersonic speeds.
IRVE – 2009-2012Two successful Inflatable Reentry Vehicle Experiments (IRVE) proved the capability of inflatable heat shield technology and opened the door for larger iterations.
LOFTID – 2022The Low Earth Orbit Flight Test of an Inflatable Decelerator (LOFTID) followed in the footsteps of its predecessor IRVE with a larger aeroshell that could be deployed to a scale much larger than the shroud. The 2022 successful test of this technology further proved the capability of HIAD technology.
MEDLI 1 and 2: 2012 & 2020As a part of the Mars Science Laboratory (MSL) mission, NASA Langley’s Mars Entry, Descent and Landing Instrument (MEDLI) was designed to gather data from the MSL entry vehicle’s heatshield during its entry and descent to the surface of Mars. MEDLI2 expanded on that groundbreaking data during the Mars 2020 mission which safely landed the Perseverance rover after successfully entering the planet’s arid atmosphere, and enabling improvements on the design for future entry systems.
Curiosity RoverCuriosity was the largest and most capable rover ever sent to Mars when it launched in 2011. Leading up the mission, Langley engineers performed millions of simulations of the entry, descent and landing phase — or the so-called “Seven Minutes of Terror” — that determines success or failure. Curiosity continues to look for signs that Mars once was – or still is – a habitable place for life as we know it.
CLPS: 2023 – PresentThe Commercial Lunar Payload Services initiative takes the Artemis mission further by working with commercial partners to advance the technology needed to return humans to the Moon and enable humanity to explore Mars.
NDLNavigation Doppler Lidar (NDL) technology, developed at Langley Research Center, uses lasers to assist spacecraft in identifying safe locations to land. In 2024, NDL flew on the Intuitive Machines’ uncrewed Nova-C lander, with its laser instruments designed to measure velocity and altitude to within a few feet. While NASA planetary landers have traditionally relied on radar and used radio waves, NDL technology has proven more accurate and less heavy, both major benefits for cost and space savings as we continue to pursue planetary missions.
SCALPSSLike Lunar Orbiter and the Viking missions before it, Stereo Cameras for Lunar Plume Surface Studies (SCALPSS) set out to better understand the surface of another celestial body. These cameras affixed to the bottom of a lunar lander focus on the interaction between the lander’s rocket plumes and the lunar surface. The SCALPSS 1.1 instrument captured first-of-its-kind imagery as the engine plumes of Firefly’s Blue Ghost lander reached the Moon’s surface. These images will serve as key pieces of data as trips to the Moon increase in the coming years.
About the AuthorAngelique Herring Share Details Last Updated Apr 03, 2025 EditorAngelique HerringContactJoseph Scott Atkinsonjoseph.s.atkinson@nasa.govLocationNASA Langley Research Center Related Terms Explore More 4 min read NASA Cameras on Blue Ghost Capture First-of-its-Kind Moon Landing Footage Article 3 weeks ago 4 min read Six NASA Instruments Will Fly to Moon on Intuitive Machines Lander Article 1 year ago 4 min read Impact Story: Navigation Doppler Lidar Article 2 years ago 7 min read Langley’s Contributions to Artemis Article 3 years ago 1 min read 2024 Annual Report Highlights Langley’s Wonder at Work Article 2 months ago 12 min read 60 Years Ago: NASA Approves the Lunar Orbiter Program Article 2 years ago Keep Exploring Discover More Topics From NASAMissions
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NASA Makes Progress on Advanced Drone Safety Management System
4 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) A Massachusetts Institute of Technology Lincoln Laboratory pilot controls a drone during NASA’s In-Time Aviation Safety Management System test series in collaboration with a George Washington University team July 17-18, 2024, at the U.S. Army’s Fort Devens in Devens, Massachusetts. MIT Lincoln Laboratory/Jay CouturierFrom agriculture and law enforcement to entertainment and disaster response, industries are increasingly turning to drones for help, but the growing volume of these aircraft will require trusted safety management systems to maintain safe operations.
NASA is testing a new software system to create an improved warning system – one that can predict hazards to drones before they occur. The In-Time Aviation Safety Management System (IASMS) will monitor, assess, and mitigate airborne risks in real time. But making sure that it can do all that requires extensive experimentation to see how its elements work together, including simulations and drone flight tests.
“If everything is going as planned with your flight, you won’t notice your in-time aviation safety management system working,” said Michael Vincent, NASA acting deputy project manager with the System-Wide Safety project at NASA’s Langley Research Center in Hampton, Virginia. “It’s before you encounter an unusual situation, like loss of navigation or communications, that the IASMS provides an alert to the drone operator.”
The team completed a simulation in the Human-Autonomy Teaming Laboratory at NASA’s Ames Research Center in California’s Silicon Valley on March 5 aimed at finding out how critical elements of the IASMS could be used in operational hurricane relief and recovery.
During this simulation, 12 drone pilots completed three 30-minute sessions where they managed up to six drones flying beyond visual line of sight to perform supply drops to residents stranded after a severe hurricane. Additional drones flew scripted search and rescue operations and levee inspections in the background. Researchers collected data on pilot performance, mission success, workload, and perceptions of the experiences, as well as the system’s usability.
This simulation is part of a longer-term strategy by NASA to advance this technology. The lessons learned from this study will help prepare for the project’s hurricane relief and recovery flight tests, planned for 2027.
As an example of this work, in the summer of 2024 NASA tested its IASMS during a series of drone flights in collaboration with the Ohio Department of Transportation in Columbus, Ohio, and in a separate effort, with three university-led teams.
For the Ohio Department of Transportation tests, a drone flew with the NASA-developed IASMS software aboard, which communicated back to computers at NASA Langley. Those transmissions gave NASA researchers input on the system’s performance.
Students from the Ohio State University participate in drone flights during NASA’s In-Time Aviation Safety Management System test series in collaboration with the Ohio Department of Transportation from March to July 2024 at the Columbus Aero Club in Ohio. NASA/Russell GilabertNASA also conducted studies with The George Washington University (GWU), the University of Notre Dame, and Virginia Commonwealth University (VCU). These occurred at the U.S. Army’s Fort Devens in Devens, Massachusetts with GWU; near South Bend, Indiana with Notre Dame; and in Richmond, Virginia with VCU. Each test included a variety of types of drones, flight scenarios, and operators.
Students from Virginia Commonwealth University walk toward a drone after a flight as part of NASA’s In-Time Aviation Safety Management System (IASMS) test series July 16, 2024, in Richmond, Virginia. NASA/Dave BowmanEach drone testing series involved a different mission for the drone to perform and different hazards for the system to avoid. Scenarios included, for example, how the drone would fly during a wildfire or how it would deliver a package in a city. A different version of the NASA IASMS was used to fit the scenario depending on the mission, or depending on the flight area.
Students from the University of Notre Dame prepare a small drone for takeoff as part of NASA’s In-Time Aviation Safety Management System (IASMS) university test series, which occurred on August 21, 2024 in Notre Dame, Indiana.University of Notre Dame/Wes EvardWhen used in conjunction with other systems such as NASA’s Unmanned Aircraft System Traffic Management, IASMS may allow for routine drone flights in the U.S. to become a reality. The IASMS adds an additional layer of safety for drones, assuring the reliability and trust if the drone is flying over a town on a routine basis that it remains on course while avoiding hazards along the way.
“There are multiple entities who contribute to safety assurance when flying a drone,” Vincent said. “There is the person who’s flying the drone, the company who designs and manufactures the drone, the company operating the drone, and the Federal Aviation Administration, who has oversight over the entire National Airspace System. Being able to monitor, assess and mitigate risks in real time would make the risks in these situations much more secure.”
All of this work is led by NASA’s System-Wide Safety project under the Airspace Operations and Safety program in support of the agency’s Advanced Air Mobility mission, which seeks to deliver data to guide the industry’s development of electric air taxis and drones.
Share Details Last Updated Apr 02, 2025 EditorDede DiniusContactTeresa Whitingteresa.whiting@nasa.gov Related Terms Explore More 3 min read NASA Supports Wildland Fire Technology Demonstration Article 2 hours ago 13 min read University Student Research Challenge (USRC) Awards Article 5 hours ago 5 min read NASA Langley’s Legacy of Landing Article 9 hours ago Keep Exploring Discover More Topics From NASAArmstrong Flight Research Center
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Artemis Astronauts & Orion Leadership Visit NASA Ames
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) Astronauts Victor Glover and Christina Koch tour the Arc Jet Facility at NASA’s Ames Research Center, learning more about the testing equipment’s capabilities to analyze thermal protection systems from George Raiche, thermophysics facilities branch chief at Ames.NASA/Donald RicheyAs NASA prepares to send astronauts to the Moon aboard the Orion spacecraft, research, testing, and development at NASA’s Ames Research Center in California’s Silicon Valley has played a critical role.
Recently, Ames welcomed Artemis II astronauts Christina Koch and Victor Glover and Orion leaders Debbie Korth, deputy program manager, and Luis Saucedo, deputy crew and service module manager, to tour Ames facilities that support the Orion Program and celebrate the achievements of employees.
The group started their visit at the Arc Jet Complex, where researchers use extremely hot, high-speed gases to simulate the intense heat of atmospheric reentry before visiting the Sensors & Thermal Protection Systems Advanced Research Laboratories. The team works to develop sensors and flight instrumentation that measure heat shield response throughout a mission.
These systems were used to develop and test Orion’s thermal protection system to ensure the safety of astronauts during future missions. After the successful return of the Artemis I Orion spacecraft, Ames research was essential when analyzing unexpected charring loss on the heat shield.
Debbie Korth, Orion deputy program manager, presents awards to the Ames workforce at the Orion Circle of Excellence Awards Ceremony, while astronauts Christina Koch and Victor Glover look on.NASA/Donald RicheyThe visit culminated in an award ceremony to honor employees with outstanding performance and a legacy of service to the Orion Program. Thirty-two employees were honored for their individual or team contributions.
“The Ames workforce has played an important role in developing, testing, and validating the Orion spacecraft’s thermal protection system as well as supporting its software and guidance, navigation, and control,” said Eugene Tu, NASA Ames center director. “I’m pleased to see their contributions recognized and celebrated by program leadership and two of the astronauts whose safety and success were in mind when ensuring these systems are safe, reliable, and the highest quality possible.”
Share Details Last Updated Apr 03, 2025 Related Terms Explore More 5 min read NASA Langley’s Legacy of Landing Article 9 hours ago 4 min read NASA Makes Progress on Advanced Drone Safety Management System Article 1 day ago 2 min read What Are the Dangers of Going to Space? We Asked a NASA Expert: Episode 55 Article 1 day ago Keep Exploring Discover More Topics From NASAAmes Research Center
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What Are the Dangers of Going to Space? We Asked a NASA Expert: Episode 55
2 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater)What are the dangers of going to space?
For human spaceflight, the first thing I think about is the astronauts actually strapping themselves to a rocket. And if that isn’t dangerous enough, once they launch and they’re out into space in deep exploration, we have to worry about radiation.
Radiation is coming at them from all directions. From the Sun, we have solar particles. We have galactic cosmic rays that are all over in the universe. And those cause damage to DNA. On Earth here, we use sunscreen to protect us from DNA damage. Our astronauts are protected from the shielding that’s around them in the space vehicles.
We also have to worry about microgravity. So what happens there? We see a lot of bone and muscle loss in our astronauts. And so to prevent this, we actually have the astronauts exercising for hours every day. And of course we don’t want to run out of food on a space exploration mission. So we want to make sure that we have everything that the astronauts need to take with them to make sure that we can sustain them.
There are many risks associated with human space exploration. NASA has been planning for these missions to make our astronauts return home safely.
[END VIDEO TRANSCRIPT]
Share Details Last Updated Apr 02, 2025 Related Terms Explore More 2 min read Artemis Astronauts & Orion Leadership Visit NASA Ames Article 5 hours ago 3 min read NASA Continues Support for Private Astronaut Missions to Space Station Article 9 hours ago 2 min read Citizen Scientists Use NASA Open Science Data to Research Life in SpaceHow can life thrive in deep space? The Open Science Data Repository Analysis Working Groups invite…
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NASA Sets Coverage for Crew Launch to Join Station Expedition 72/73
NASA astronaut Jonny Kim will launch aboard the Roscosmos Soyuz MS-27 spacecraft to the International Space Station, accompanied by cosmonauts Sergey Ryzhikov and Alexey Zubritsky, where they will join the Expedition 72/73 crew in advancing scientific research.
Kim, Ryzhikov, and Zubritsky will lift off at 1:47 a.m. EDT Tuesday, April 8 (10:47 a.m. Baikonur time) from the Baikonur Cosmodrome in Kazakhstan.
Watch live launch and docking coverage on NASA+. Learn how to watch NASA content through a variety of platforms.
After a two-orbit, three-hour trajectory to the station, the spacecraft will dock automatically to the station’s Prichal module at approximately 5:03 a.m. Shortly after, hatches will open between Soyuz and the space station.
Once aboard, the trio will join NASA astronauts Nichole Ayers, Anne McClain, and Don Pettit, JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi, and Roscosmos cosmonauts Alexey Ovchinin, Kirill Peskov, and Ivan Vagner.
NASA’s coverage is as follows (all times Eastern and subject to change based on real-time operations):
Tuesday, April 8
12:45 a.m. – Launch coverage begins on NASA+.
1:47 a.m. – Launch
4:15 a.m. – Rendezvous and docking coverage begins on NASA+.
5:03 a.m. – Docking
7 a.m. – Hatch opening and welcome remarks coverage begins on NASA+.
7:20 a.m. – Hatch opening
The trio will spend approximately eight months aboard the orbital laboratory as Expedition 72 and 73 crew members before returning to Earth in December. This will be the first flight for Kim and Zubritsky, and the third for Ryzhikov.
For more than two decades, 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 focus on providing human space transportation services and destinations as part of a robust low Earth orbit economy, NASA is focusing more 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:
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X-ray Clues Reveal Destroyed Planet
This image of the Helix Nebula, released on March 4, 2025, shows a potentially destructive white dwarf at the nebula’s center: this star may have destroyed a planet. This has never been seen before – and could explain a mysterious X-ray signal that astronomers have detected from the nebula for over 40 years.
This view combines X-rays from NASA’s Chandra X-ray Observatory (magenta), optical light data from NASA’s Hubble Space Telescope (orange, light blue), infrared data from the European Southern Observatory VISTA telescope (gold, dark blue), and ultraviolet data from GALEX (purple) of the Helix Nebula. Data from Chandra indicates that this white dwarf has destroyed a very closely orbiting planet.
Image credit: X-ray: NASA/CXC/SAO/Univ Mexico/S. Estrada-Dorado et al.; Ultraviolet: NASA/JPL; Optical: NASA/ESA/STScI (M. Meixner)/NRAO (T.A. Rector); Infrared: ESO/VISTA/J. Emerson; Image Processing: NASA/CXC/SAO/K. Arcand
NASA Continues Support for Private Astronaut Missions to Space Station
3 min read
Preparations for Next Moonwalk Simulations Underway (and Underwater) The International Space Station is pictured from the SpaceX Dragon spacecraft by a Crew-8 member shortly after undocking from the Harmony module’s space-facing port as the orbital outpost was soaring 272 miles above the cloudy Patagonia region of South America.NASANASA is seeking proposals for two new private astronaut missions to the International Space Station, targeted for 2026 and 2027, as the agency continues its commitment to expanding access to space. These private missions enable American commercial companies to further develop capabilities and support a continuous human presence in low Earth orbit.
“We are in an incredible time for human spaceflight, with more opportunities to access space and grow a thriving commercial economy in low Earth orbit,” said Dana Weigel, program manager for the International Space Station at NASA’s Johnson Space Center in Houston. “NASA remains committed to supporting this expansion by leveraging our decades of expertise to help industry gain the experience needed to train and manage crews, conduct research, and develop future destinations. Private astronaut missions are a key part of this effort, providing companies with hands-on opportunities to refine their capabilities and build partnerships that will shape the future of low Earth orbit.”
The new flight opportunities will be the fifth and sixth private astronaut missions to the orbiting laboratory coordinated by NASA. The first three missions were accomplished by Axiom Space in April 2022, May 2023, and January 2024, with a fourth scheduled for no earlier than May 2025.
Each of the new missions may be docked to the space station for up to 14 days. Specific dates depend on spacecraft traffic at the space station and in-orbit activity planning and constraints. Private astronaut missions must be brokered by a U.S. entity and use U.S. transportation spacecraft that meet NASA’s International Space Station visiting vehicle requirements, policies, and procedures. For additional details, refer to Focus Area 4A of NASA Research Announcement (NRA) NNJ13ZBG001N.
Proposals are due by 5 p.m. EDT on Friday, May 30, 2025.
For solicitation information, visit:
https://www.nasa.gov/johnson/jsc-procurement/pam
For more than two decades, people have lived and worked continuously aboard the International Space Station, advancing scientific knowledge and demonstrating new technologies, making research breakthroughs 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 focus on providing human space transportation services and destinations as part of a robust low Earth orbit economy, NASA’s Artemis campaign is underway at the Moon, where the agency is preparing for future human exploration of Mars.
Learn more about the International Space Station at:
Keep Exploring Discover More TopicsLow Earth Orbit Economy
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Lagniappe for April 2025
Explore Lagniappe for April 2025 featuring:
- NASA-Sponsored FIRST Robotics Welcomes Teams to Magnolia Regional
- NASA Leaders Visit Representatives
- Blood Moon in South Mississippi
New beginnings feel a lot like the month of April. It is the heart of spring and the season that symbolizes growth and renewal.
April is the perfect time to break free from old routines and try something new.
If you have landed here in this website corner of our digital world, consider this your open invitation to continue ahead on the journey with NASA Stennis by following us on social media.
It is time to say goodbye to the Lagniappe publication as we know it, but do not worry. All of the great news about the center and its frontline activities still will be available, just in a new way – via our social media platforms! Gator wants you to feel more connected than ever as we continue to help power space dreams in south Mississippi. Moving forward, join NASA Stennis in our digital playground for even more of that extra-something special.
This playground is not limited to only fun, or making new friends, or learning new stuff.
Whether you are on Facebook, Instagram, YouTube, or X, there is a place, and space, for all of that and more.
As we close out the website edition of NASA Stennis Lagniappe, we turn the page and look forward to new possibilities ahead.
Let’s keep building one connection at a time because here at America’s largest rocket propulsion test site, it is more than just content.
It is where the NASA Stennis team will continue building on its proven expertise in all areas of work, and where you will have a front row seat to experience it unfold.
So, click the links below to become a NASA Stennis follower today. Then, invite your friends to become followers as well.
Facebook logo @NASAStennis @NASAStennis Instagram logo @NASAStennis NASA Stennis Top News NASA-Sponsored FIRST Robotics Welcomes Teams to Magnolia Regional NASA serves as a lead sponsor, along with NASA Stennis employees and interns volunteering, for the third annual FIRST Robotics Magnolia Regional Competition on March 14. The event in Laurel, Mississippi, welcomed 37 teams from eight states (Alabama, California, Florida, Louisiana, Minnesota, Missouri, Mississippi, and Tennessee) and one team from Mexico. The FIRST (For the Inspiration and Recognition of Science and Technology) Robotics event joined NASA’s Robotics Alliance Project to combine the excitement of sport with the rigors of science, technology, engineering, and mathematics (STEM) in field games using industrial-sized robots.NASA/Danny Nowlin NASA serves as a lead sponsor, along with NASA Stennis employees and interns volunteering, for the third annual FIRST Robotics Magnolia Regional Competition on March 14. The event in Laurel, Mississippi, welcomed 37 teams from eight states (Alabama, California, Florida, Louisiana, Minnesota, Missouri, Mississippi, and Tennessee) and one team from Mexico. The FIRST (For the Inspiration and Recognition of Science and Technology) Robotics event joined NASA’s Robotics Alliance Project to combine the excitement of sport with the rigors of science, technology, engineering, and mathematics (STEM) in field games using industrial-sized robots.NASA/Danny Nowlin NASA serves as a lead sponsor, along with NASA Stennis employees and interns volunteering, for the third annual FIRST Robotics Magnolia Regional Competition on March 14. The event in Laurel, Mississippi, welcomed 37 teams from eight states (Alabama, California, Florida, Louisiana, Minnesota, Missouri, Mississippi, and Tennessee) and one team from Mexico. The FIRST (For the Inspiration and Recognition of Science and Technology) Robotics event joined NASA’s Robotics Alliance Project to combine the excitement of sport with the rigors of science, technology, engineering, and mathematics (STEM) in field games using industrial-sized robots.NASA/Danny Nowlin NASA serves as a lead sponsor, along with NASA Stennis employees and interns volunteering, for the third annual FIRST Robotics Magnolia Regional Competition on March 14. The event in Laurel, Mississippi, welcomed 37 teams from eight states (Alabama, California, Florida, Louisiana, Minnesota, Missouri, Mississippi, and Tennessee) and one team from Mexico. The FIRST (For the Inspiration and Recognition of Science and Technology) Robotics event joined NASA’s Robotics Alliance Project to combine the excitement of sport with the rigors of science, technology, engineering, and mathematics (STEM) in field games using industrial-sized robots.NASA/Danny Nowlin NASA serves as a lead sponsor, along with NASA Stennis employees and interns volunteering, for the third annual FIRST Robotics Magnolia Regional Competition on March 14. The event in Laurel, Mississippi, welcomed 37 teams from eight states (Alabama, California, Florida, Louisiana, Minnesota, Missouri, Mississippi, and Tennessee) and one team from Mexico. The FIRST (For the Inspiration and Recognition of Science and Technology) Robotics event joined NASA’s Robotics Alliance Project to combine the excitement of sport with the rigors of science, technology, engineering, and mathematics (STEM) in field games using industrial-sized robots.NASA/Danny Nowlin NASA serves as a lead sponsor, along with NASA Stennis employees and interns volunteering, for the third annual FIRST Robotics Magnolia Regional Competition on March 14. The event in Laurel, Mississippi, welcomed 37 teams from eight states (Alabama, California, Florida, Louisiana, Minnesota, Missouri, Mississippi, and Tennessee) and one team from Mexico. The FIRST (For the Inspiration and Recognition of Science and Technology) Robotics event joined NASA’s Robotics Alliance Project to combine the excitement of sport with the rigors of science, technology, engineering, and mathematics (STEM) in field games using industrial-sized robots.NASA/Danny Nowlin NASA serves as a lead sponsor, along with NASA Stennis employees and interns volunteering, for the third annual FIRST Robotics Magnolia Regional Competition on March 14. The event in Laurel, Mississippi, welcomed 37 teams from eight states (Alabama, California, Florida, Louisiana, Minnesota, Missouri, Mississippi, and Tennessee) and one team from Mexico. The FIRST (For the Inspiration and Recognition of Science and Technology) Robotics event joined NASA’s Robotics Alliance Project to combine the excitement of sport with the rigors of science, technology, engineering, and mathematics (STEM) in field games using industrial-sized robots.NASA/Danny Nowlin NASA serves as a lead sponsor, along with NASA Stennis employees and interns volunteering, for the third annual FIRST Robotics Magnolia Regional Competition on March 14. The event in Laurel, Mississippi, welcomed 37 teams from eight states (Alabama, California, Florida, Louisiana, Minnesota, Missouri, Mississippi, and Tennessee) and one team from Mexico. The FIRST (For the Inspiration and Recognition of Science and Technology) Robotics event joined NASA’s Robotics Alliance Project to combine the excitement of sport with the rigors of science, technology, engineering, and mathematics (STEM) in field games using industrial-sized robots.NASA/Danny Nowlin NASA serves as a lead sponsor, along with NASA Stennis employees and interns volunteering, for the third annual FIRST Robotics Magnolia Regional Competition on March 14. The event in Laurel, Mississippi, welcomed 37 teams from eight states (Alabama, California, Florida, Louisiana, Minnesota, Missouri, Mississippi, and Tennessee) and one team from Mexico. The FIRST (For the Inspiration and Recognition of Science and Technology) Robotics event joined NASA’s Robotics Alliance Project to combine the excitement of sport with the rigors of science, technology, engineering, and mathematics (STEM) in field games using industrial-sized robots.NASA/Danny Nowlin NASA serves as a lead sponsor, along with NASA Stennis employees and interns volunteering, for the third annual FIRST Robotics Magnolia Regional Competition on March 14. The event in Laurel, Mississippi, welcomed 37 teams from eight states (Alabama, California, Florida, Louisiana, Minnesota, Missouri, Mississippi, and Tennessee) and one team from Mexico. The FIRST (For the Inspiration and Recognition of Science and Technology) Robotics event joined NASA’s Robotics Alliance Project to combine the excitement of sport with the rigors of science, technology, engineering, and mathematics (STEM) in field games using industrial-sized robots.NASA/Danny Nowlin Center Activities NASA Leaders Visit Representatives U.S. Sen. Cindy Hyde-Smith of Mississippi, center, greets NASA Stennis Deputy Director Christine Powell, right, and NASA Stennis Legislative Affairs Officer and Chief of Staff Troy Frisbie on March 4. Powell and Frisbie visited with Smith and other congressional members in conjunction with the recent NASA Artemis Suppliers Conference in Washington, D.C.NASA/Stennis U.S. Sen. Roger Wicker of Mississippi welcomes NASA Stennis Deputy Director Christine Powell and other guests on March 5. Powell visited Wicker in conjunction with the NASA Artemis Suppliers Conference in Washington, D.C.NASA/Stennis U.S. Rep. Mike Ezell of Mississippi, fourth from right, stands with acting NASA Kennedy Space Center Director Kelvin Manning, fifth from right; NASA Stennis Deputy Director Christine Powell, third from right; NASA Stennis Legislative Affairs Officer and Chief of Staff Troy Frisbie, far left; and several congressional staff members March 5. The NASA officials visited with Ezell and other congressional members in conjunction with the recent NASA Artemis Suppliers Conference in Washington, D.C.NASA/Stennis NASA Space Flight Awareness Program Recognizes Stennis EmployeesNASA’s Stennis Space Center employees were recognized with Honoree Awards from NASA’s Space Flight Awareness Program during a March 10 ceremony in Orlando, Florida, for outstanding support of human spaceflight.
Read More about Space Flight Awareness Honorees Blood Moon in South Mississippi Images show the total lunar eclipse, known as a Blood Moon, over south Mississippi during the early morning hours of March 14. A lunar eclipse occurs when the Sun, Earth, and Moon align so that the Moon passes into Earth’s shadow. In a total lunar eclipse, the entire Moon falls within the darkest part of Earth’s shadow, called the umbra. When the Moon is within the umbra, it appears red-orange. Lunar eclipses are sometimes called “Blood Moons” because of this phenomenon.NASA/Rebecca Mataya Images show the total lunar eclipse, known as a Blood Moon, over south Mississippi during the early morning hours of March 14. A lunar eclipse occurs when the Sun, Earth, and Moon align so that the Moon passes into Earth’s shadow. In a total lunar eclipse, the entire Moon falls within the darkest part of Earth’s shadow, called the umbra. When the Moon is within the umbra, it appears red-orange. Lunar eclipses are sometimes called “Blood Moons” because of this phenomenon.NASA/Rebecca Mataya Images show the total lunar eclipse, known as a Blood Moon, over south Mississippi during the early morning hours of March 14. A lunar eclipse occurs when the Sun, Earth, and Moon align so that the Moon passes into Earth’s shadow. In a total lunar eclipse, the entire Moon falls within the darkest part of Earth’s shadow, called the umbra. When the Moon is within the umbra, it appears red-orange. Lunar eclipses are sometimes called “Blood Moons” because of this phenomenon.NASA/Rebecca Mataya Images show the total lunar eclipse, known as a Blood Moon, over south Mississippi during the early morning hours of March 14. A lunar eclipse occurs when the Sun, Earth, and Moon align so that the Moon passes into Earth’s shadow. In a total lunar eclipse, the entire Moon falls within the darkest part of Earth’s shadow, called the umbra. When the Moon is within the umbra, it appears red-orange. Lunar eclipses are sometimes called “Blood Moons” because of this phenomenon.NASA/Rebecca Mataya Images show the total lunar eclipse, known as a Blood Moon, over south Mississippi during the early morning hours of March 14. A lunar eclipse occurs when the Sun, Earth, and Moon align so that the Moon passes into Earth’s shadow. In a total lunar eclipse, the entire Moon falls within the darkest part of Earth’s shadow, called the umbra. When the Moon is within the umbra, it appears red-orange. Lunar eclipses are sometimes called “Blood Moons” because of this phenomenon.NASA/Rebecca Mataya Images show the total lunar eclipse, known as a Blood Moon, over south Mississippi during the early morning hours of March 14. A lunar eclipse occurs when the Sun, Earth, and Moon align so that the Moon passes into Earth’s shadow. In a total lunar eclipse, the entire Moon falls within the darkest part of Earth’s shadow, called the umbra. When the Moon is within the umbra, it appears red-orange. Lunar eclipses are sometimes called “Blood Moons” because of this phenomenon.NASA/Rebecca Mataya Learn More About the Blood Moon U.S. Senator’s Staff Visit NASA Stennis NASA’s Stennis Space Center hosts staff members of U.S. Sen. Roger Wicker of Mississippi on March 21 for a site visit. Pictured (left to right) are Kelly McCarthy, NASA Stennis partnership development lead; Troy Frisbie, NASA Stennis legislative affairs officer and chief of staff; Jason Richard, NASA Stennis propulsion business manager; Joe Schuyler, director of the NASA Stennis Engineering and Test Directorate; Emily Yetter, Wicker’s military legislative assistant; Dan Hillenbrand, Wicker’s legislative director; Terry Miller, U.S. Navy Fellow assigned to Wicker’s office; NASA Stennis Associate Director Rodney McKellip; Duane Armstrong, manager of the NASA Stennis Strategic Business Development Office; Drew Parks, Navy Senate liaison officer to Wicker’s office. The members representing the Mississippi senator’s staff toured NASA Stennis, including the Thad Cochran Test Stand, where NASA Stennis is preparing for future Artemis testing.NASA/Danny Nowlin NASA Stennis Hosts Leadership Class Approximately 50 members of the Leadership Hancock Class of 2025 visit NASA Stennis on March 26 for a full-day tour that included meeting NASA Stennis leaders and seeing center facilities, such as the Thad Cochran Test Stand pictured in the background. Leadership Hancock is an annual program by the Hancock County Chamber of Commerce designed to identify and cultivate future community leaders.NASA/Danny Nowlin NASA Stennis Interns Tour Site NASA student interns stand in the flame deflector at the Fred Haise Test Stand on March 7 during a NASA Stennis site tour. Interns include (left to right): Addison Mitchell (Pathways intern for Engineering and Test Directorate); Andrew Evans (Office of STEM Engagement intern for Autonomous Systems Lab); Mikayla Chandler (Office of STEM Engagement intern for ASTRO CAMP Community Partners); and Kristen Zack (Office of STEM Engagement intern for Autonomous Systems Lab). NASA Office of STEM Engagement paid internships allow high school and college-level students to contribute to agency projects under the guidance of a NASA mentor. The Pathways program offers current students and recent graduates paid internships that can be direct pipelines to full-time employment at NASA upon graduation.NASA/Danny Nowlin Rocket Test Group Visits NASA StennisNASA Stennis partnered with Mississippi Enterprise for Technology to host more than 100 members of the 57th Rocket Test Group on March 18-19.
The group toured the south Mississippi NASA center on March 19, learning how NASA Stennis operates as NASA’s primary, and America’s largest, rocket propulsion test site to serve the nation and commercial sector with its unique capabilities and expertise.
Read More about Rocket Test Groups Visit NASA in the NewsNASA’s Artemis II Orion Service Module Buttoned Up for Launch – NASA
Welcome Home! NASA’s SpaceX Crew-9 Back on Earth After Science Mission – NASA
NASA Science Continues After Firefly’s First Moon Mission Concludes – NASA
NASA Artemis II Core Stage Goes Horizontal Ahead of Final Integration – NASA
Employee Profile: Rebecca Mataya Rebecca Mataya is a budget analyst at NASA’s Stennis Space Center. “Whether you are an engineer, analyst, lawyer, technician, communicator or innovator, there is a place for you here at NASA,” she said. “Every skill contributes to the greater mission of pushing the boundaries of exploration, discovery, and progress. If you have a passion, determination, and willingness to learn, NASA is a place where you can grow and leave a lasting impact on the future of space.”NASA/StennisA career path can unfold in unexpected ways. Ask NASA’s Rebecca Mataya. The journey to NASA’s Stennis Space Center near Bay St. Louis, Mississippi, was not planned but “meant to be,” she said.
Read More About Rebecca Mataya Additional Resources Explore More 4 min read Lagniappe for January 2025 Article 3 months ago 3 min read Lagniappe for February 2025 Article 2 months ago 4 min read Lagniappe for March 2025 Article 4 weeks agoNASA Space Flight Awareness Program Recognizes Stennis Employees
NASA’s Stennis Space Center employees were recognized with Honoree Awards from NASA’s Space Flight Awareness Program during a March 10 ceremony in Orlando, Florida, for outstanding support of human spaceflight.
Stennis Space Center employee Melissa Wagner of Pass Christian, Mississippi, is presented with the NASA Space Flight Awareness Program Honoree Award during a March 10 ceremony. Wagner (second from left) receives the award from (left to right): NASA astronaut Randy Bresnik, NASA Exploration Systems Development Mission Directorate Acting Associate Administrator Dr. Lori Glaze, and NASA Space Operations Mission Directorate Associate Administrator Kenneth Bowersox. NASA/Kennedy Space CenterMelissa Wagner of Pass Christian, Mississippi, is a NASA contract specialist in the Office of Procurement at NASA Stennis. She received the honor for contributions to NASA’s Artemis campaign by identifying potential risks related to propulsion test efforts in support of the initiative, resulting in successful mitigation actions.
NASA’s Stennis Space Center employee Samone Wilson of Hattiesburg, Mississippi, is presented with the NASA Space Flight Awareness Program Honoree Award during a March 10 ceremony. Wilson (second from left) receives the award from (left to right): NASA astronaut Randy Bresnik, NASA Space Operations Mission Directorate Associate Administrator Kenneth Bowersox, and NASA Exploration Systems Development Mission Directorate Acting Associate Administrator Dr. Lori Glaze.NASA/Kennedy Space CenterSamone Wilson of Hattiesburg, Mississippi, is a NASA public affairs specialist in the Office of Communications at NASA Stennis. She received the honor for her work in telling others about NASA and NASA Stennis activities and missions.
Timothy Miller of Pearl River, Louisiana, is a senior drafter for Syncom Space Services at NASA Stennis. Although unable to attend the ceremony, he received the honor for contributions supporting flight systems integration, facility readiness, and cost reduction with his use of Creo Parametric modeling, a powerful 3D software.
Madison Monti of Kiln, Mississippi, is a security support specialist for Chenega Global Protection at NASA Stennis. Although unable to attend the ceremony, she received the honor for contributions supporting the badging office at NASA Stennis to ensure a consistent, efficient, and secure process.
NASA astronaut Randy Bresnik, Space Operations Mission Directorate Associate Administrator Kenneth Bowersox, and Exploration Systems Development Mission Directorate Acting Associate Administrator Dr. Lori Glaze presented the awards.
Bresnik, assistant-to-the-chief of the Astronaut Office for Exploration, was selected as a NASA astronaut in 2004. He manages the development and testing of everything that will operate beyond low-Earth orbit on Artemis missions. Bresnik previously served as commander of the International Space Station for Expedition 53 and flight engineer for Expedition 52.
In recognition of flight program contributions, honorees toured NASA’s Kennedy Space Center in Florida and viewed the SpaceX Dragon spacecraft named Endurance in conjunction with the launch of NASA’s SpaceX Crew-10.
The spacecraft carried NASA astronauts Anne McClain and Nichole Ayers, JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi, and Roscomos cosmonaut Kirill Pesko to the International Space Station on March 14 as part of NASA’s Commercial Crew Program. NASA’s Space Flight Awareness Program recognizes outstanding job performances and contributions by civil service and contract employees throughout the year and focuses on excellence in quality and safety in support of human spaceflight. The Honoree Award is one of the highest honors presented to employees for their dedication to quality work and flight safety. Recipients must have contributed beyond their normal work requirements toward achieving a particular human spaceflight program goal; contributed to a major cost savings; been instrumental in developing material that increases reliability, efficiency or performance; assisted in operational improvements; or been a key player in developing a beneficial process improvement.
For information about Silver Snoopy and other Space Flight Awareness awards, visit:
For information about NASA’s Stennis Space Center, visit:
Rocket Test Group Visits NASA Stennis
NASA Stennis partnered with Mississippi Enterprise for Technology to host more than 100 members of the 57th Rocket Test Group on March 18-19.
NASA Stennis partnered with Mississippi Enterprise for Technology to host more than 100 members of the 57th Rocket Test Group on March 18-19.NASA/Jason RichardThe group toured the south Mississippi NASA center on March 19, learning how NASA Stennis operates as NASA’s primary, and America’s largest, rocket propulsion test site to serve the nation and commercial sector with its unique capabilities and expertise.
NASA Stennis partnered with Mississippi Enterprise for Technology to host more than 100 members of the 57th Rocket Test Group on March 18-19.NASA/Jason RichardThe day included tours of test stands and facilities hosted by NASA Stennis test complex personnel. Visits included the Fred Haise Test Stand, where NASA Stennis tests RS-25 engines to help power NASA’s Artemis missions to the Moon and beyond; the Thad Cochran Test Stand, where NASA Stennis will test NASA’s exploration upper stage for future Artemis missions; the E Test Complex, where NASA Stennis supports agency and commercial propulsion test activity; and the L3Harris Technologies (formerly Aerojet Rocketdyne) Engine Assembly Facility, where RS-25 engines are produced.
NASA Stennis partnered with Mississippi Enterprise for Technology to host more than 100 members of the 57th Rocket Test Group on March 18-19.NASA/Jason RichardThe group also received overviews from site personnel on the Rocket Propulsion Test Program Office located at NASA Stennis, on lessons learned from testing at the E Test Complex, and on the NASA Data Acquisition System developed onsite.
NASA Stennis partnered with Mississippi Enterprise for Technology to host more than 100 members of the 57th Rocket Test Group on March 18-19.NASA/Jason RichardThe Rocket Test Group originally formed in response to a congressional demand for an ongoing working group crossing agency and company boundaries. It is a volunteer organization intended to allow rocket test facility operators to come together to recommend solutions for difficult testing problems; lower testing costs by reducing time spent on solving critical issues and eliminating duplicate programs; facilitate the activation of new facilities; learn from each other by viewing different methods and touring various facilities; provide a networking opportunity for testing advice and problem solving support; and allow test facility operators to stay informed on the newest developments.
NASA Stennis partnered with Mississippi Enterprise for Technology to host more than 100 members of the 57th Rocket Test Group on March 18-19.L3Harris TechnologiesNASA Webb Explores Effect of Strong Magnetic Fields on Star Formation
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Follow-up research on a 2023 image of the Sagittarius C stellar nursery in the heart of our Milky Way galaxy, captured by NASA’s James Webb Space Telescope, has revealed ejections from still-forming protostars and insights into the impact of strong magnetic fields on interstellar gas and the life cycle of stars.
“A big question in the Central Molecular Zone of our galaxy has been, if there is so much dense gas and cosmic dust here, and we know that stars form in such clouds, why are so few stars born here?” said astrophysicist John Bally of the University of Colorado Boulder, one of the principal investigators. “Now, for the first time, we are seeing directly that strong magnetic fields may play an important role in suppressing star formation, even at small scales.”
Detailed study of stars in this crowded, dusty region has been limited, but Webb’s advanced near-infrared instruments have allowed astronomers to see through the clouds to study young stars like never before.
“The extreme environment of the galactic center is a fascinating place to put star formation theories to the test, and the infrared capabilities of NASA’s James Webb Space Telescope provide the opportunity to build on past important observations from ground-based telescopes like ALMA and MeerKAT,” said Samuel Crowe, another principal investigator on the research, a senior undergraduate at the University of Virginia and a 2025 Rhodes Scholar.
Bally and Crowe each led a paper published in The Astrophysical Journal.
Image A: Milky Way Center (MeerKAT and Webb) An image of the Milky Way captured by the MeerKAT (formerly the Karoo Array Telescope) radio telescope array puts the James Webb Space Telescope’s image of the Sagittarius C region in context. Like a super-long exposure photograph, MeerKAT shows the bubble-like remnants of supernovas that exploded over millennia, capturing the dynamic nature of the Milky Way’s chaotic core. At the center of the MeerKAT image the region surrounding the Milky Way’s supermassive black hole blazes bright. Huge vertical filamentary structures echo those captured on a smaller scale by Webb in Sagittarius C’s blue-green hydrogen cloud.NASA, ESA, CSA, STScI, SARAO, Samuel Crowe (UVA), John Bally (CU), Ruben Fedriani (IAA-CSIC), Ian Heywood (Oxford) Image B: Milky Way Center (MeerKAT and Webb), Labeled The star-forming region Sagittarius C, captured by the James Webb Space Telescope, is about 200 light-years from the Milky Way’s central supermassive black hole, Sagittarius A*. The spectral index at the lower left shows how color was assigned to the radio data to create the image. On the negative end, there is non-thermal emission, stimulated by electrons spiraling around magnetic field lines. On the positive side, thermal emission is coming from hot, ionized plasma. For Webb, color is assigned by shifting the infrared spectrum to visible light colors. The shortest infrared wavelengths are bluer, and the longer wavelengths appear more red.NASA, ESA, CSA, STScI, SARAO, Samuel Crowe (UVA), John Bally (CU), Ruben Fedriani (IAA-CSIC), Ian Heywood (Oxford) Using Infrared to Reveal Forming StarsIn Sagittarius C’s brightest cluster, the researchers confirmed the tentative finding from the Atacama Large Millimeter Array (ALMA) that two massive stars are forming there. Along with infrared data from NASA’s retired Spitzer Space Telescope and SOFIA (Stratospheric Observatory for Infrared Astronomy) mission, as well as the Herschel Space Observatory, they used Webb to determine that each of the massive protostars is already more than 20 times the mass of the Sun. Webb also revealed the bright outflows powered by each protostar.
Even more challenging is finding low-mass protostars, still shrouded in cocoons of cosmic dust. Researchers compared Webb’s data with ALMA’s past observations to identify five likely low-mass protostar candidates.
The team also identified 88 features that appear to be shocked hydrogen gas, where material being blasted out in jets from young stars impacts the surrounding gas cloud. Analysis of these features led to the discovery of a new star-forming cloud, distinct from the main Sagittarius C cloud, hosting at least two protostars powering their own jets.
“Outflows from forming stars in Sagittarius C have been hinted at in past observations, but this is the first time we’ve been able to confirm them in infrared light. It’s very exciting to see, because there is still a lot we don’t know about star formation, especially in the Central Molecular Zone, and it’s so important to how the universe works,” said Crowe.
Magnetic Fields and Star FormationWebb’s 2023 image of Sagittarius C showed dozens of distinctive filaments in a region of hot hydrogen plasma surrounding the main star-forming cloud. New analysis by Bally and his team has led them to hypothesize that the filaments are shaped by magnetic fields, which have also been observed in the past by the ground-based observatories ALMA and MeerKAT (formerly the Karoo Array Telescope).
“The motion of gas swirling in the extreme tidal forces of the Milky Way’s supermassive black hole, Sagittarius A*, can stretch and amplify the surrounding magnetic fields. Those fields, in turn, are shaping the plasma in Sagittarius C,” said Bally.
The researchers think that the magnetic forces in the galactic center may be strong enough to keep the plasma from spreading, instead confining it into the concentrated filaments seen in the Webb image. These strong magnetic fields may also resist the gravity that would typically cause dense clouds of gas and dust to collapse and forge stars, explaining Sagittarius C’s lower-than-expected star formation rate.
“This is an exciting area for future research, as the influence of strong magnetic fields, in the center of our galaxy or other galaxies, on stellar ecology has not been fully considered,” said Crowe.
The James Webb Space Telescope is the world’s premier space science observatory. Webb is solving mysteries in our solar system, looking beyond to distant worlds around other stars, and probing the mysterious structures and origins of our universe and our place in it. Webb is an international program led by NASA with its partners, ESA (European Space Agency) and CSA (Canadian Space Agency).
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View/Download all image products at all resolutions for this article from the Space Telescope Science Institute.
View/Download the science paper led by Bally from the The Astrophysical Journal.
View/Download the science paper led by Crowe from the The Astrophysical Journal.
Media ContactsLaura Betz – laura.e.betz@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Leah Ramsay – lramsay@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
Christine Pulliam – cpulliam@stsci.edu
Space Telescope Science Institute, Baltimore, Md.
Read more: press releases about the center of the Milky Way
NASA’s Universe of Learning: ViewSpace Interactive image tour of the center of the Milky Way
Learn more about the Milky Way and Sagittarius Constellation
Related For Kids En Español Keep Exploring Related Topics James Webb Space TelescopeWebb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
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Share Details Last Updated Apr 02, 2025 EditorMarty McCoyContactLaura Betzlaura.e.betz@nasa.gov Related TermsCitizen Scientists Use NASA Open Science Data to Research Life in Space
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Citizen Scientists Use NASA Open Science Data to Research Life in Space 2023 Workshop of Analysis Working Group members, Washington, D.C., November 14, 2023. Now, you are invited to join their quest to understand how life can thrive in deep space! Want to learn more first? Join our live virtual event April 17 at 3pm Eastern Time to hear an overview of the OSDR AWG’s operations. Photo: NASA OSDR TeamHow can life thrive in deep space? The Open Science Data Repository Analysis Working Groups invite volunteers from all backgrounds to help answer this question. Request to join these citizen science groups to help investigate how life adapts to space environments, exploring topics like radiation effects, microgravity’s impact on human and plant health, and how microbes change in orbit.
Currently, nine Analysis Working Groups (AWGs) hold monthly meetings to advance their specific focus areas. Participants collaborate using an online platform, the AWG “Forum-Space”, where they connect with peers and experts, join discussions, and contribute to over 20 active projects.
The AWGs work with data primarily from the NASA Open Science Data Repository (OSDR), a treasure trove of spaceflight data on physiology, molecular biology, bioimaging, and much more. For newcomers, there are tutorials and a comprehensive paper covering all aspects of the repository and the AWG community. You can explore 500+ studies, an omics multi-study visualization portal, the environmental data app, and RadLab, a portal for radiation telemetry data. (“Omics” refers to fields of biology that end in “omics,” like “genomics”.)
Each of the nine AWGs has a Lead who organizes their group and holds monthly virtual meetings. Once you join, make sure to connect with the Lead and get on the agenda so you can introduce yourself. Learn more about the AWGs here.
Have an idea for a new project? Propose a new project and help lead it! From data analysis and visualization to shaping data standards and conducting literature meta-analyses, there’s a place for everyone to contribute. Request to join, and together, we can address a great challenge for humanity: understanding and enabling life to thrive in deep space!
Want to learn more?On April 17 at 3pm Eastern Time, the NASA Citizen Science Leaders Series is hosting an virtual event with Ryan Scott about these Analysis Working Groups and their work. Ryan is the Science Lead for the Ames Life Sciences Data Archive and the liaison between the Open Data Science Repository and the Analysis Working Groups. Click here to register for this event!
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