The Soyuz MS-27 spacecraft is seen as it lands in a remote area near the town of Zhezkazgan, Kazakhstan on Dec. 9, 2025, with Expedition 73 NASA astronaut Jonny Kim, and Roscosmos cosmonauts Sergey Ryzhikov and Alexey Zubritsky aboard.
The trio returned to Earth after logging 245 days in space as members of Expeditions 72 and 73 aboard the International Space Station. While aboard the orbiting laboratory, Kim contributed to a wide range of scientific investigations and technology demonstrations.
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.
A flash of lightning, and then—something else. High above a storm, a crimson figure blinks in and out of existence. If you see it, you are a lucky witness of a sprite, one of the least-understood electrical phenomena in Earth’s upper atmosphere.
Sprites occur at some 50 miles (80 kilometers) altitude, high above thunderstorms. They appear moments after a lightning strike – a sudden reddish flash that can take a range of shapes, often combining diffuse plumes and bright, spiny tendrils. Some sprites tend to dance over the storms, turning on and off one after another. Many questions about how and why they form remain unanswered. Sprites are the most frequently observed type of Transient Luminous Events (TLEs); TLEs can take a variety of fanciful shapes with equally fanciful names.
This image is the NASA Science Calendar Image of the Month for December 2025. Learn more about sprites and download this photo to use as a wallpaper on your phone or computer.
Galaxy clusters are the most massive objects in the universe held together by gravity, containing up to several thousand individual galaxies and huge reservoirs of superheated, X-ray-emitting gas. The mass of this hot gas is typically about five times higher than the total mass of all the galaxies in galaxy clusters. In addition to these visible components, 80% of the mass of galaxy clusters is supplied by dark matter. These cosmic giants are bellwethers not only for the galaxies, stars and black holes within them, but also for the evolution and growth of the universe itself.
It is no surprise then that NASA’s Chandra X-ray Observatory has observed many galaxy clusters over the lifetime of the mission. Chandra’s X-ray vision allows it to see the enormous stockpiles of hot cluster gas, with temperatures as high as 100 million degrees, with exquisite clarity. This blazing gas tells stories about past and present activity within galaxy clusters.
X-ray: NASA/CXC/Univ. of Chicago/H. McCall; Image processing: NASA/CXC/SAO/N. Wolk
Many of these galaxy clusters host supermassive black holes at their centers, which periodically erupt in powerful outbursts. These explosions generate jets that are visible in radio wavelengths, which inflate bubbles full of energetic particles; these bubbles carry energy out into the surrounding gas. Chandra’s images have revealed a wealth of other structures formed during these black hole outbursts, including hooks, rings, arcs, and wings. However, appearances alone don’t tell us what these structures are or how they formed.
To tackle this problem, a team of astronomers developed a novel image-processing technique to analyze X-ray data, allowing them to identify features in the gas of galaxy clusters like never before, classifying them by their nature rather than just their appearance. Prior to this technique, which they call “X-arithmetic,” scientists could only identify the nature of some of the features and in a much less efficient way, via studies of the amounts of X-ray energy dispersed at different wavelengths. The authors applied X-arithmetic to 15 galaxy clusters and galaxy groups (these are similar to galaxy clusters but with fewer member galaxies). By comparing the outcome from the X-arithmetic technique to computer simulations, researchers now have a new tool that will help in understanding the physical processes inside these important titans of the universe.
A new paper looks at how these structures appear in different parts of the X-ray spectrum. By splitting Chandra data into lower-energy and higher-energy X-rays and comparing the strengths of each structure in both, researchers can classify them into three distinct types, which they have colored differently. A pink color is given to sound waves and weak shock fronts, which arise from pressure disturbances traveling at close to the speed of sound, compressing the hot gas into thin layers. The bubbles inflated by jets are colored yellow, and cooling or slower-moving gas is blue. The resulting images, “painted” to reflect the nature of each structure, offer a new way to interpret the complex aftermath of black hole activity using only X-ray imaging data. This method works not only on Chandra (and other X-ray) observations, but also on simulations of galaxy clusters, providing a tool to bridge data and theory.
The images in this new collection show the central regions of five galaxy clusters in the sample: MS 0735+7421, the Perseus Cluster, and M87 in the Virgo Cluster in the top row and Abell 2052 and Cygnus A on the bottom row. All of these objects have been released to the public before by the Chandra X-ray Center, but this is the first time this special technique has been applied. The new treatment highlights important differences between the galaxy clusters and galaxy groups in the study.
The galaxy clusters in the study often have large regions of cooling or slow-moving gas near their centers, and only some show evidence for shock fronts. The galaxy groups, on the other hand, are different. They show multiple shock fronts in their central regions and smaller amounts of cooling and slow-moving gas compared to the sample of galaxy clusters.
This contrast between galaxy clusters and galaxy groups suggests that black hole feedback — that is, the interdependent relationship between outbursts from a black hole and its environment — appears stronger in galaxy groups. This may be because feedback is more violent in the groups than in the clusters, or because a galaxy group has weaker gravity holding the structure together than a galaxy cluster. The same outburst from a black hole, with the same power level, can therefore more easily affect a galaxy group than a galaxy cluster.
There are still many open questions about these black hole outbursts. For example, scientists would like to know how much energy they put into the gas around them and how often they occur. These violent events play a key role in regulating the cooling of the hot gas and controlling the formation of stars in clusters. By revealing the physics underlying the structures they leave behind, the X-arithmetic technique brings us closer to understanding the influence of black holes on the largest scales.
A paper describing this new technique and its results has been published in The Astrophysical Journal and is led by Hannah McCall from the University of Chicago. The other authors are Irina Zhuravleva (University of Chicago), Eugene Churazov (Max Planck Institute for Astrophysics, Germany), Congyao Zhang (University of Chicago), Bill Forman and Christine Jones (Center for Astrophysics | Harvard & Smithsonian), and Yuan Li (University of Massachusetts at Amherst).
NASA’s Marshall Space Flight Center in Huntsville, Alabama, manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
NASA Begins Moon Mission Plume-Surface Interaction Tests
Views of the 60-foot vacuum sphere in the which the plume-surface interaction testing is happening.
Credits: NASA/Joe Atkinson
In March, NASA researchers employed a new camera system to capture data imagery of the interaction between Firefly Aerospace Blue Ghost Mission-1 lander’s engine plumes and the lunar surface.
Through NASA’s Artemis campaign, this data will help researchers understand the hazards that may occur when a lander’s engine plumes blast away at the lunar dust, soil, and rocks.
The data also will be used by NASA’s commercial partners as they develop their human landing systems to safely transport astronauts from lunar orbit to the Moon’s surface and back, beginning with Artemis III.
To better understand the science of lunar landings, a team at NASA’s Langley Research Center in Hampton, Virginia, has initiated a series of plume-surface interaction tests inside a massive 60-foot spherical vacuum chamber.
This plume-surface interaction ground test is the most complex test of its kind to be undertaken in a vacuum chamber
Ashley Korzun
PSI Testing Lead at NASA Langley
“This plume-surface interaction ground test is the most complex test of its kind to be undertaken in a vacuum chamber,” said Ashley Korzun, testing lead at NASA Langley. “If I’m in a spacecraft and I’m going to move all that regolith while landing, some of that’s going to hit my lander. Some of it’s going to go out toward other things — payloads, science experiments, eventually rovers and other assets. Understanding those physics is pivotal to ensuring crew safety and mission success.”
The campaign, which will run through spring of 2026, should provide an absolute treasure trove of data that researchers will be able to use to improve predictive models and influence the design of space hardware. As Korzun mentioned, it’s a big undertaking, and it involves multiple NASA centers, academic institutions, and commercial entities both small and large.
Korzun’ s team will test two types of propulsion systems in the vacuum sphere. For the first round of tests this fall, they are using an ethane plume simulation system designed by NASA’s Stennis Space Center near Bay St. Louis, Mississippi, and built and operated by Purdue University in West Lafayette, Indiana. The ethane system generates a maximum of about 100 pounds of thrust — imagine the force necessary to lift or support a 100-pound person. It heats up but doesn’t burn.
A view of the ethane nozzle researchers are using during the first phase of testing. NASA/Wesley Chambers
After completing the ethane tests, the second round of tests will involve a 14-inch, 3D-printed hybrid rocket motor developed at Utah State University in Logan, Utah, and recently tested at NASA’s Marshall Space Flight Center in Huntsville, Alabama. It produces around 35 pounds of thrust, igniting both solid propellant and a stream of gaseous oxygen to create a hot, powerful stream of rocket exhaust, simulating a real rocket engine but at smaller scale for this test series.
Researchers will test both propulsion systems at various heights, firing them into a roughly six-and-a-half-foot diameter, one-foot-deep bin of simulated lunar regolith, called Black Point-1 that has jagged, cohesive properties similar to lunar regolith.
“It gives us a huge range of test conditions,” Korzun said, “to be able to talk about spacecraft of all different kinds going to the Moon, and for us to understand what they’re going to do as they land or try to take back off from the surface.”
Researchers will use this 14-inch, 3D-printed hybrid rocket motor during the second phase of testing.
The data from these tests at NASA Langley will be critical in developing and validating models to predict the effects of plume surface interaction for landing on the Moon and even Mars, ensuring mission success for the HLS landers and the safety of our astronauts
Daniel Stubbs
Engineer with HLS Plume and Aero Environments Team at NASA Marshall
Korzun sees this test campaign as more than a one-shot, Moon-specific thing. The entire operation is modular by design and can also prepare NASA for missions to Mars. The lunar regolith simulant can be replaced with a Mars simulant that’s more like sand. Pieces of hardware and instrumentation can be unbolted and replaced to represent future Mars landers. Rather than take the vacuum sphere down to really low pressure like on the Moon, it can be adjusted to a pressure that simulates the atmosphere on the Red Planet. “Mars has always been in our road maps,” Korzun said.
But for now, the Moon looms large.
A number of instruments, including SCALPSS cameras similar to the ones that captured imagery of the plume-surface interaction between Firefly Aerospace’s Blue Ghost lander and the Moon in March, will capture data on the sphere tests.
NASA/Ryan Hill
“This test campaign is one of the most flight-relevant and highly instrumented plume-surface interaction test series NASA has ever conducted,” said Daniel Stubbs, an engineer with the human landing systems plume and aero environments team at NASA Marshall. “The data from these tests at NASA Langley will be critical in developing and validating models to predict the effects of plume-surface interaction for landing on the Moon and even Mars, ensuring mission success for the human landing systems and the safety of our astronauts.”
Through the Artemis campaign, NASA will send astronauts to explore the Moon for scientific discovery, economic benefits, and to build upon our foundation for the first crewed missions to Mars – for the benefit of all.
Preparations for Next Moonwalk Simulations Underway (and Underwater)
NASA engineer Hanbong Lee demonstrates capabilities to manage busy urban airspace traffic during a recent simulation at NASA’s Ames Research Center in California’s Silicon Valley.
NASA/Brandon Torres-Navarrete
NASA is helping shape the future of urban air travel with a new simulation that will manage how electric air taxis and drones can successfully operate within busy areas.
The demonstration, held at NASA’s Ames Research Center in California’s Silicon Valley earlier this year, focused on a system called the Strategic Deconfliction Simulation, which helps coordinate flight plans before takeoff, reducing the risk of conflicts in busy urban environments
At the event, researchers demonstrated NASA’s Situational Viewer and Demand-Capacity Balancing Monitor, which visualizes air traffic and adjusts flight plans in real time. The simulation demonstrated traffic scenarios involving drone operations throughout the Dallas-Fort Worth area, testing how preplanned flights could improve congestion and manage the demand and capacity of the airspace – ensuring that all aircraft can operate smoothly even in crowded conditions.
Working with industry partners is critical to NASA’s efforts to develop and refine technologies needed for future air mobility. During the simulation, the company, ANRA Technologies, demonstrated its fleet and vertiport management systems, which are designed to support the coordination of multiple aircraft and ground operations.
“Simulating these complex environments supports broader efforts to ensure safe integration of drones and other advanced vehicles into the US airspace,” said Hanbong Lee, engineer at NASA Ames. “By showcasing these capabilities, we’re delivering critical data and lessons learned to support efforts at NASA and industry.”
This demonstration is another step toward the NASA team’s plan to hold a technical capability level simulation in 2026. This upcoming simulation would help shape the development of services aimed at managing aircraft flying in urban areas.
The simulation was created through a NASA team from its Air Mobility Pathfinders project, part of the agency’s continuing work to find solutions for safely integrating innovative new aircraft such as air taxis into U.S. cities and the national airspace. By developing advanced evaluations and simulations, the project supports safe, scalable, and publicly trusted air travel in urban areas, paving the way for a future where air taxis and drones are a safe and reliable part of everyday life.
A pilot signals to a crew member before takeoff from NASA’s Armstrong Flight Research Center in Edwards, California, on Aug. 21, 2025. Accompanying him in the high-flying ER-2 aircraft is one of the most advanced imaging spectrometers in the solar system.
NASA/Christopher LC Clark
Called AVIRIS-5, it’s the latest in a long line of sensors pioneered by NASA JPL to survey Earth, the Moon, and other worlds.
Cradled in the nose of a high-altitude research airplane, a new NASA sensor has taken to the skies to help geoscientists map rocks hosting lithium and other critical minerals on Earth’s surface some 60,000 feet below. In collaboration with the U.S. Geological Survey (USGS), the flights are part of the largest airborne campaign of its kind in the country’s history.
But that’s just one of many tasks that are on the horizon for AVIRIS-5, short for Airborne Visible/Infrared Imaging Spectrometer-5, which has a lot in common with sensors used to explore other planets.
NASA’s AVIRIS flies aboard a research plane in this animation, detecting minerals on the ground such as hectorite — a lithium-bearing clay — by the unique patterns of light that they reflect. The different wavelengths, measured in nanometers, look like colorful squiggles in the box on the right. Credit: NASA’s Conceptual Image Lab
About the size of a microwave oven, AVIRIS-5 detects the spectral “fingerprints” of minerals and other compounds in reflected sunlight. Like its cousins flying in space, the sensor takes advantage of the fact that all kinds of molecules, from rare earth elements to flower pigments, have unique chemical structures that absorb and reflect different wavelengths of light.
The technology was pioneered at NASA’s Jet Propulsion Laboratory in Southern California in the late 1970s. Over the decades, imaging spectrometers have visited every major rocky body in the solar system from Mercury to Pluto. They’ve traced Martian crust in full spectral detail, revealed lakes on Titan, and tracked mineral-rich dust across the Sahara and other deserts. One is en route to Europa, an ocean moon of Jupiter, to search for the chemical ingredients needed to support life.
Image cubes illustrate the volume of data returned by JPL imaging spectrometers. The front panel shows roads and fields around Tulare, California, as seen by AVIRIS-5 during a checkout flight earlier this year. The side panels depict the spectral fingerprint captured for every point in the image.
NASA/JPL-Caltech
Another imaging spectrometer, NASA’s Moon Mineralogy Mapper, was the first to discover water on the lunar surface in 2009. “That dataset continues to drive our investigations as we look for in situ resources on the Moon” as part of NASA’s Artemis campaign, said Robert Green, a senior research scientist at NASA JPL who’s contributed to multiple spectroscopy missions across the solar system.
Prisms, black silicon
While imaging spectrometers vary depending on their mission, they have certain hardware in common — including mirrors, detector arrays, and electron-beam gratings — designed to capture light shimmering off a surface and then separate it into its constituent colors, like a prism.
Light-trapping black silicon is one of the darkest materials ever fabricated. The technology is standard for JPL’s ultraprecise imaging spectrometers.
NASA/JPL-Caltech
Many of the best-in-class imaging spectrometers flying today were made possible by components invented at NASA JPL’s Microdevices Laboratory. Instrument-makers there combine breakthroughs in physics, chemistry, and material science with the classical properties of light discovered by physicist Isaac Newton in the 17th century. Newton’s prism experiments revealed that visible light is composed of a rainbow of colors.
Today, NASA JPL engineers work with advanced materials such as black silicon — one of the darkest substances ever manufactured — to push performance. Under a powerful microscope, black silicon looks like a forest of spiky needles. Etched by lasers or chemicals, the nanoscale structures prevent stray light from interfering with the sample by trapping it in their spikes.
Treasure hunting
The optical techniques used at the Microdevices Laboratory have advanced continuously since the first AVIRIS instrument took flight in 1986. Four generations of these sensors have now hit the skies, analyzing erupting volcanoes, diseased crops, ground zero debris in New York City, and wildfires in Alabama, among many other deployments. The latest model, AVIRIS-5, features spatial resolution that’s twice as fine as that of its predecessor and can resolve areas ranging from less than a foot (30 centimeters) to about 30 feet (10 meters).
So far this year, it has logged more than 200 hours of high-altitude flights over Nevada, California, and other Western states as part of a project called GEMx (Geological Earth Mapping Experiment). The flights are conducted using NASA’s ER-2 aircraft, operated out of the agency’s Armstrong Flight Research Center in Edwards, California. The effort is the airborne component of a larger USGS initiative, called Earth Mapping Resources Initiative (Earth MRI), to modernize mapping of the nation’s surface and subsurface.
The NASA and USGS team has, since 2023, gathered data over more than 366,000 square miles (950,000 square kilometers) of the American West, where dry, treeless expanses are well suited to mineral spectroscopy.
An exciting early finding is a lithium-bearing clay called hectorite, identified in the tailings of an abandoned mine in California, among other locations. Lithium is one of about 50 minerals at risk of supply chain disruption that USGS has deemed critical to national security and the economy.
Helping communities capture new value from old and abandoned prospects is one of the long-term aspirations of GEMx, said Dana Chadwick, an Earth system scientist at NASA JPL. So is identifying sources of acid mine drainage, which can occur when waste rocks weather and leach into the environment.
“The breadth of different questions you can take on with this technology is really exciting, from land management to snowpack water resources to wildfire risk,” Chadwick said. “Critical minerals are just the beginning for AVIRIS-5.”
More about GEMx
The GEMx research project is expected to last four years and is funded by the USGS Earth MRI, through investments from the Bipartisan Infrastructure Law. The initiative will capitalize on both the technology developed by NASA for spectroscopic imaging, as well as the expertise in analyzing the datasets and extracting critical mineral information from them.
The Soyuz MS-27 spacecraft is seen as it lands in a remote area near the town of Zhezkazgan, Kazakhstan, with Expedition 73 NASA astronaut Jonny Kim, and Roscosmos cosmonauts Sergey Ryzhikov, and Alexey Zubritsky aboard, Dec. 9, 2025.
NASA/Bill Ingalls
NASA astronaut Jonny Kim returned to Earth on Tuesday alongside Roscosmos cosmonauts Sergey Ryzhikov and Alexey Zubritsky, wrapping up an eight-month science mission aboard the International Space Station to benefit life on Earth and future space exploration.
They made a safe, parachute-assisted landing at 12:03 a.m. EST (10:03 a.m. local time), southeast of Dzhezkazgan, Kazakhstan, after departing the space station at 8:41 p.m. on Dec. 8, aboard the Soyuz MS-27 spacecraft.
Over the course of 245 days in space, the crew orbited Earth 3,920 times, traveling nearly 104 million miles. They launched to the space station on April 8. This mission marked the first spaceflight for both Kim and Zubritsky, while Ryzhikov completed his third journey to space, logging a total of 603 days in space.
NASA astronaut Jonny Kim shows off the Matroyshka (stacking) doll he received upon his return to Earth, Dec. 9, 2025. Kim and his crewmates landed safely aboard their Soyuz MS-27 spacecraft in a remote area near the town of Zhezkazgan, Kazakhstan.
NASA
While aboard the orbiting laboratory, Kim contributed to a wide range of scientific investigations and technology demonstrations. He studied the behavior of bioprinted tissues containing blood vessels in microgravity for an experiment helping advance space-based tissue production to treat patients on Earth. He also evaluated the remote command of multiple robots in space for the Surface Avatar study, which could support the development of robotic assistants for future exploration missions. Additionally, Kim worked on developing in-space manufacturing of DNA-mimicking nanomaterials, which could improve drug delivery technologies and support emerging therapeutics and regenerative medicine.
Following post-landing medical checks, the crew will return to the recovery staging area in Karaganda, Kazakhstan. Kim will then board a NASA aircraft bound for the agency’s Johnson Space Center in Houston.
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:
Michelle Hoehn is a cost accountant at NASA’s Stennis Space Center, where her work contributes to NASA’s Artemis program that will send astronauts to the Moon to prepare for future human exploration of Mars.
NASA/Danny Nowlin
Michelle Hoehn vividly remembers the day a seed was planted for her future at NASA’s Stennis Space Center near Bay St. Louis, Mississippi.
As a seventh grader, the Bogalusa, Louisiana, native joined her dad for Father/Daughter Day at NASA Stennis. Hoehn knew she wanted to be part of something bigger, something that sparked wonder and purpose, in the moment she visited her dad’s office. She recalled feeling a sense of awe and possibility that day.
It was not until her second year at Southeastern Louisiana University – after the birth of her first child – that she focused on building a career, though. Finance and accounting have always been a part of her life. She filed paperwork at her grandfather’s store and helped her mom during tax season.
“It was clear that this field was the right fit for me,” she said.
Today, Hoehn works as a cost accountant in the Office of the Chief Financial Officer at NASA Stennis. She ensures all costs are accurately recorded and reported. Her work supports financial integrity, enabling informed decisions and efficient use of resources.
“It is incredibly rewarding to know that my work helps keep NASA’s operations transparent and efficient because every accurate number supports the bigger mission of space exploration and discovery,” said Hoehn.
Hoehn’s financial management work supports NASA’s Artemis program that will send astronauts to the Moon to establish a sustainable presence and prepare for future human exploration of Mars.
“I’m honored to be a part of NASA’s Artemis effort,” she said. “Knowing that my work helps enable the next chapter of lunar exploration, and ultimately the journey to Mars, is both humbling and deeply motivating.”
One of the most fascinating parts of Hoehn’s work at NASA Stennis is seeing how even the smallest financial details can have a ripple effect on major NASA missions.
Although her work is often behind the scenes, the data she manages helps guide decisions that impact propulsion testing, technology development, and even future space exploration.
“It is incredible to realize that a spreadsheet I work on today could be tied to a rocket engine test of the future,” she said. “That connection between everyday tasks and extraordinary outcomes is something I never take for granted, and it is what makes working at NASA Stennis so rewarding.”
Working as an accountant on large, complex projects – some worth millions of dollars – also comes with challenges.
The projects demand precision, attention to detail, and a deep understanding of evolving financial regulations and systems. To stay ahead, Hoehn keeps an open mind and embraces continuous learning. She is always looking for ways to grow, adapt, and strengthen her role in supporting NASA’s financial integrity and broader mission.
This year marks 15 years as a NASA employee for Hoehn and 21 years of service overall at NASA Stennis, where she began as a contractor in 2004.
“The workforce at NASA Stennis is highly collaborative and mission-driven,” Hoehn said. “Whether you are working in engineering, finance, or support services, there is a collective sense of purpose and pride in contributing to space exploration and scientific discovery. It is an environment where ideas are welcomed, excellence is encouraged, and every individual plays a vital role in the success of NASA’s mission.”
From the time Hoehn walked in her dad’s office as a seventh-grade student, she has experienced firsthand the opportunities NASA Stennis offers.
“NASA Stennis is a place of unlimited potential, not only in its contributions to NASA’s missions, but in the opportunities it offers to current and future employees, customers, and stakeholders,” Hoehn said. “It is where I have been empowered to exceed the goals I once set for myself and continue to grow, both personally and professionally. NASA Stennis is a place where you are encouraged to be part of something greater than yourself.”
This composite image of the Cassiopeia A (or Cas A) supernova remnant, released Jan. 8, 2024, contains X-rays from Chandra (blue), infrared data from Webb (red, green, blue), and optical data from Hubble (red and white). A study by the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft has made the first-ever X-ray detections of chlorine and potassium in the wreckage.
X-ray: NASA/CXC/SAO; Optical: NASA/ESA/STScI; IR: NASA/ESA/CSA/STScI/Milisavljevic et al., NASA/JPL/CalTech; Image Processing: NASA/CXC/SAO/J. Schmidt and K. Arcand
The Cassiopeia A supernova remnant glows in X-ray, visible, and infrared light in this Jan. 8, 2024, image that combines data from NASA’s Chandra X-ray Observatory and Hubble, Webb, and Spitzer space telescopes. A study by the XRISM (X-ray Imaging and Spectroscopy Mission) spacecraft has made the first-ever X-ray detections of chlorine and potassium from the wreckage; a paper about the result was published Dec. 4, 2025, in Nature Astronomy.
By the time the Artemis II Orion spacecraft launches to the Moon next year, its many components will already have traveled thousands of miles and moved across multiple facilities before coming together at NASA’s Kennedy Space Center. Branelle Rodriguez, Artemis II vehicle manager for the Orion Program, has overseen many parts of that journey. Her job is to ensure the spacecraft is ready for its historic mission – carrying humans to the Moon for the first time in over 50 years.
Branelle Rodriguez crouches inside an Orion spacecraft training unit aboard the USS San Diego in March 2024. The training unit was used during a full recovery simulation with the Artemis II crew.
Image courtesy of Branelle Rodriguez
Based at NASA’s Johnson Space Center in Houston, Rodriguez has been involved in every stage of the spacecraft’s lifecycle – from development and production through testing and final launch readiness. Her program-level leadership focuses on ensuring the spacecraft’s hardware and subsystems are integrated and flight-ready. Most recently, she collaborated closely with Exploration Ground Systems at Kennedy to oversee the spacecraft’s move to the Vehicle Assembly Building, where it was mated with NASA’s SLS (Space Launch System) rocket. “We are getting our teams trained and ready so that we are GO for the Artemis II mission,” she said.
Her 21-year NASA career spans numerous roles at Johnson. She started in the center’s Engineering Directorate, developing and building life support and habitation hardware for the Space Shuttle Program and the International Space Station Program. She went on to lead teams of engineers and flight controllers tasked with real-time resolution of anomalies aboard the International Space Station before transitioning to the Orion Program in 2022.
“Looking back, every role I’ve held, every team I’ve been a part of, and every milestone we’ve achieved together has been truly remarkable,” she said. “I’m incredibly proud to have played a part in it all.”
Rodriguez has been fascinated by space since she was a little girl. “Growing up in northern Minnesota, I was lucky to experience the beauty of clear, starlit skies on a regular basis,” she recalled. When Rodriguez was a teenager, her family encouraged her to attend Space Academy in Huntsville, Alabama, where she participated in mock astronaut training, flight controller simulations, and hands-on engineering projects. “It was a pivotal experience that only deepened my passion for space exploration.”
Branelle Rodriguez stands in front of the Artemis II Orion spacecraft as it completes processing in the Multi-Payload Processing Facility at NASA’s Kennedy Space Center in Florida.
Image courtesy of Branelle Rodriguez
Rodriguez applied to NASA’s internship program while studying mechanical engineering at the University of North Dakota. She was not accepted, but she did not give up. She spent a semester interning at Dow Chemical to gain more experience while continuing to apply for internships across multiple NASA centers. “On my eighth attempt, I was accepted at Johnson,” she said. Three internships and one graduation later, Rodriguez landed a full-time position in the Engineering Directorate’s Crew and Thermal Systems Division. “It’s been an incredible journey—and a dream realized,” she said.
As a student athlete, Rodriguez knew the importance of teamwork from a young age, but said its value really became clear after joining NASA. “Some goals take time. There will be setbacks and struggles, but when you stick together, you build the kind of trust and relationships that are the foundation for long-term success,” she said. “That’s exactly what NASA represents. We take on some of the most complex and ambitious challenges imaginable—and we do it as a team.”
She added, “Especially now, it’s more important than ever to remember what we’re capable of when we work together, and to celebrate the wins—big or small—because each one brings us closer to the extraordinary.”
Rodriguez also appreciates having a team outside of the office. One of the greatest challenges she has faced is balancing the demands of a fulfilling, high-impact career with the needs of her family. “Like many parents, there are days when everything feels in sync, and days when I know I’ve fallen short,” she said, acknowledging that she must continually adapt to shifting needs and prioritize tasks to remain focused on what matters most at any given moment. “I’m beyond grateful for my family,” she said. “They are my foundation, and they truly understand and support my passion for the work I do. Without their love, and the broader village that helps make it all possible, I wouldn’t be where I am today.”
Branelle Rodriguez, her husband Scott, and her children Samantha and Brooks in the Mission Control Center at Johnson Space Center during the Artemis I mission in 2022. The family had an opportunity to ask the Artemis I Orion spacecraft questions via the Callisto technology demonstration carried aboard the 25-day mission.
Image courtesy of Branelle Rodriguez
To her children and future generations, Rodriguez hopes to pass on a desire to keep exploring. “As humans, we are naturally driven to grow, learn, and push beyond our limits,” she said. “Space exploration is still in its early stages when viewed through the lens of history, and the achievements of the next generation will be truly extraordinary. I want them to carry forward the curiosity, courage, and determination needed to reach new frontiers and unlock the unknown.”
