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The Marshall Star for January 31, 2024


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The Marshall Star for January 31, 2024

a full-duration, 500-second hot fire of an RS-25 certification engine Jan. 27 in the background as seen across an empty field

Marshall Commemorates NASA’s Day of Remembrance

By Celine Smith

Team members across NASA’s Marshall Space Flight Center congregated Jan. 25 in the lobby of Building 4221 to observe NASA’s Day of Remembrance.

Each January, the agency pauses to honor members of the NASA family who lost their lives while furthering the cause of exploration and discovery, including the crews of Apollo 1 and space shuttles Challenger and Columbia.

Bill Hill, left, director of Marshall’s Safety and Mission Assurance Directorate, observes Larry Leopard, Marshall associate director, technical, lighting a candle in honor of those lost at the Day of Remembrance ceremony.
Bill Hill, left, director of Marshall’s Safety and Mission Assurance Directorate, observes Larry Leopard, Marshall associate director, technical, lighting a candle in honor of those lost at the Day of Remembrance ceremony.
NASA/Krisdon A. Manecke

The center’s ceremony included speeches from Larry Leopard, Marshall associate director, technical, and Bill Hill, director of Marshall’s Safety and Mission Assurance Directorate.

Leopard spoke about his memories of Challenger and Columbia’s influence on his work ethic at Marshall.

“With every failure and loss, it is up to those who remain to learn and grow from those who have gone on before us to prevent the same mistakes as we push on to new heights,” Leopard said.

Hill emphasized the importance of how a strong safety culture at Marshall is vital to mission success. He also encouraged Marshall team members to attend center safety workshops and complete training to eliminate as much risk as possible on future missions.

tde-0612.jpg?w=2048
From left, Shannon Segovia, Marshall’s deputy director of communications, Hill, Leopard, and acting Center Director Joseph Pelfrey gather around the ceremonial wreath and candle.
NASA/Krisdon A. Manecke

“Seventeen of our brave astronauts paid the ultimate price for our failures,” Hill said. “Learning from our experience, we must become more humble, more dedicated to doing things right, more vigilant, questioning the process at every turn.”

After their speeches, a candle was lit in memory of lives lost in the pursuit of exploration and discovery along with a moment of silence.

“The accidents we’ve had in the past are reminders of how hard, dangerous, and risky space exploration is,” acting Center Director Joseph Pelfrey said afterward. “They serve as a reminder for us to be diligent at our jobs. As we bring younger generations into the workforce, we have to continue to teach them as well so that as a community we don’t repeat these mistakes.”

Smith, a Media Fusion employee, supports the Marshall Office of Communications.

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National Mentoring Month: Troubleshooting with NASA’s Aaron Comis and Brad Solomon

By Jessica Barnett

Mentorship is a valuable partnership that benefits both mentors and mentees. Like any relationship, it also comes with its fair share of challenges.

Those challenges can include misaligned expectations, miscommunications, time constraints, lack of engagement, and burnout. Overcoming those challenges is possible, but it takes commitment, communication, and flexibility from both parties.

Official Portrait: Brad Solomon
Brad Solomon is the chief information officer in the Management of Information Technology office at Marshall Space Flight Center. Solomon signed up for the Systems Engineering Mentoring program to help younger members of NASA’s workforce as they navigate their lives and careers.
NASA/Danielle Burle

Those concepts are all too familiar to Brad Solomon and Aaron Comis, who were paired as mentor and mentee respectively. Solomon, who currently serves as chief information officer for NASA’s Marshall Space Flight Center, said he signed up for the systems engineering mentoring program and was purposefully paired with Comis, a former Pathways intern from Johnson Space Center who now works as chief digital engineer at Goddard Space Flight Center.

“We found we had more in common than we knew, as both of us were involved in the digital transformation initiative led by Jill Marlowe, and that our challenges at Marshall and Goddard in that effort were very common,” Solomon said.

Aaron Comis
Aaron Comis serves as chief digital engineer in the Engineering and Technology Directorate at Goddard Space Flight Center. Comis said mentors have been a major influence throughout his career, from his days as an intern at Johnson Space Center through today.
NASA

Being at different NASA centers meant the potential for additional challenges, but it also provided additional perspective and opportunities for the pair during their mentorship journey. As NASA wraps up its celebration of this year’s Mentoring Month, Comis and Solomon sat down to offer their insight into how mentorship has influenced their lives and careers, as well as their tips for helping things go right and their advice for when things go wrong.

Question: What does mentorship mean to you?

Comis: To me, mentorship is a judgment-free relationship between peers that provides a safe space to discuss life with a focus on relating conversation back to a specific topic, whether it be professional, educational, personal, etc. We all eat, sleep, win, lose, and face challenges. The only constant is everything relating back to life.

Solomon: As a mentor, it means inspiring and helping create the next generation of leaders who will carry on the NASA legacy. I was fortunate to be part of the construction of ISS (International Space Station) and the Space Shuttle Program support, but the days of major NASA programs at the heart of the NASA mission are largely over, given the growth of the commercial space sector. More than ever, we need an innovative workforce adept at modern engineering techniques. With over 700 new NASA employees at Marshall since the pandemic began, all of us should feel obligated to help launch their young careers.

Question: What impact has mentorship had on you and your career?

Comis: Mentors have played a huge, albeit unassuming, role throughout my career, as early as my time at Johnson Space Center as a Pathways intern. My mentors throughout the years have provided me with a safe space to ask questions that I wasn’t comfortable with asking publicly, supported me through hard times, and celebrated big wins with me. I honestly believe my career wouldn’t be as successful or fun without the many mentors who helped me along the way.

Solomon: We all can look back at our careers and see the handful of leaders and conversations that changed the trajectory and propelled our careers. I had the privilege of being part of a Boeing program in the early 1990s that provided excellent leadership training and the opportunity to hear from aerospace leaders. Jonathan Pettus and Neil Rodgers instilled project management discipline and tireless work ethics in the implementation of NASA’s first enterprise financial management systems. Being part of an enterprise IT source evaluation board gave me opportunities to work with leaders like Byron Butler and Walt Melton, who taught me how to read and appreciate precision in contracting. Without mentors like these, I would not have been prepared for promotion opportunities when they were presented.

Question: How do you handle potential conflicts or disagreements to ensure a constructive resolution?

Comis: My role at Goddard is focused on change management, which can be a challenging role. If I come across potential conflicts or disagreements, I start with self-evaluation and attempt to take a step back from the situation. Did I communicate my intended message clearly and effectively? Was it possible that the intended message wasn’t understood? If the topic was the issue, not the communication, then it helps to have trusted mentors from all walks of life. This way, there is a better chance of achieving a constructive resolution in some form. Geographic separation – for example, being at different NASA centers – also helps with discussing certain sensitive topics, since this provides an additional layer of privacy and protection for everyone and ensures objective mentorship.

Solomon: That’s such an important trait in an effective leader. First, never take any criticism or disagreement personally, even when it is delivered with animus. There are always reasons behind it, and it may not have anything to do with you. Second, set aside all emotion, and see the issue as a roadblock – first, to a successful personal relationship, then to the mission. You must address the lack of trust before you can solve the problem. Do not hesitate to insert humor and self-deprecation to reduce tension. That will make addressing trust and the issue at hand easier. Finally, always start a hard conversation by restating and affirming the validity of the other person’s position (seek first to understand). This way, you are at least on neutral ground to start the difficult conversation.

Question: How would you suggest a mentor or mentee address differing expectations?

Comis: Expectations are key to a successful mentorship and should be addressed during the very first mentor/mentee interaction, starting with, ‘Why do you want to be a mentor/mentee, and what do you hope to gain from this experience?’ This is something that I learned from my most recent formal mentorship experience that I intend on carrying forward with my future mentor/mentee relationships.

Solomon: All mentor/mentee initial meetings should start with a statement of expectations from the mentee. As mentor, do not critique the statement. Treat it as the starting point for the conversation. Mentors should listen, affirm, then add to the expectation with additional potential directions in which the discussions can go. Save additional guidance for future meetings. Instead, get to know each other. Where is the mentee in their career? What are their aspirations? Why? What do they enjoy doing outside of work? At the end of the meeting, set the mentoring agenda for the next meeting.

Question: What advice do you have for someone else who wants to find or be a mentor?

Comis: Take the plunge! Becoming a mentor or mentee can be challenging, since it involves opening yourself up, whether by asking for help or offering help to someone else’s real and ongoing challenges, but it’s also hugely rewarding. Of course, it’s important to get to know someone before unloading your problems onto them, but at a certain point, there’s only one way to continue to establish the relationship, and that’s through trust. Ideally, have multiple mentors throughout your career, some local and some who intentionally are not local. This way, for more sensitive issues, you have an added layer of separation for peace of mind. I’d recommend everyone look for someone you already trust (for a potential mentor) or someone you see or know of who might be struggling and offer a helping hand (as a potential mentor for them). You never know how additional perspective might help you overcome challenges you weren’t even aware you had!

Solomon: To the mentor: First, there is no wrong way to do this. Don’t worry about meeting an expectation. It’s best to just be yourself and be genuine. Be present in the discussions, not distracted. Reschedule if you have a scheduling conflict. It helps if there is an affinity between the mentor and mentee to begin with, so work needs to be done to effectively match the two. If you are not right for each other, terminate after the first session and take action to help find a better match. Take good notes. You might want to consider a separate notebook for the engagement, so you can look back on notes from the past session. Mentees are opening themselves to you, so be trustworthy. Remember the last conversation and bring it forward to the next one. Be willing to share about yourself as well.

To the mentee: Be honest and open. You get out only what you are willing to invest. This means you will be out of your comfort zone. Don’t worry; it’s supposed to feel uncomfortable at times. Don’t be afraid to ask questions or raise uncomfortable questions, because everyone has been at your point and gone through similar experiences in their careers. Know that your time will come when you will be the mentor – perhaps sooner than you expect.

Editor’s note: This is the third in a Marshall Star series during National Mentoring Month in January. Marshall team members can learn more about the benefits of mentoring on Inside Marshall.

Barnett, a Media Fusion employee, supports the Marshall Office of Communications.

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Marshall Team Supports Space Night with the Huntsville Havoc

NASA’s Marshall Space Flight Center joined the Huntsville Havoc for Space Night. The sold-out Jan. 26 game featured more than 4,900 fans for a themed hockey game designed to celebrate Huntsville’s robust aerospace community.

Marshall team member Michael Allen shares details about the IXPE mission with fans Jan. 26 at the Huntsville Havoc’s Space Night.
Marshall team member Michael Allen shares details about the IXPE mission with fans Jan. 26 at the Huntsville Havoc’s Space Night.
NASA/Taylor Goodwin

Thousands of space and hockey fans enjoyed exhibits and outreach provided by Marshall team members from across the center, including the Centennial Challenges Program; IXPE (Imaging X-ray Polarimetry Explorer); Technology Demonstration Missions; and SLS (Space Launch System) Program. 

Huntsville Havoc mascot, Rukus, poses in front of NASA exhibits at Space Night.
Huntsville Havoc mascot, Rukus, poses in front of NASA exhibits at Space Night.
NASA/Taylor Goodwin
Marshall team member Savannah Bullard shares details of the Centennial Challenges Program with Space Night attendees.
Marshall team member Savannah Bullard shares details of the Centennial Challenges Program with Space Night attendees.
NASA/Taylor Goodwin

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NASA Marks Halfway Point for Artemis Moon Rocket Engine Certification Series

NASA completed the sixth of 12 scheduled RS-25 engine certification tests in a critical series for future flights of the agency’s SLS (Space Launch System) rocket as engineers conducted a full-duration hot fire Jan. 27 at NASA’s Stennis Space Center.

The current series builds on previous hot fire testing conducted at NASA Stennis to help certify production of new RS-25 engines by lead contractor Aerojet Rocketdyne, an L3 Harris Technologies company. The new engines will help power NASA’s SLS rocket on future Artemis missions to the Moon and beyond, beginning with Artemis V.

a full-duration, 500-second hot fire of an RS-25 certification engine Jan. 27 in the background as seen across an empty field
NASA completed a full-duration, 500-second hot fire of an RS-25 certification engine Jan. 27, marking the halfway point in a critical test series to support future SLS (Space Launch System) missions to the Moon and beyond as NASA explores the secrets of the universe for the benefit of all.
NASA/Danny Nowlin

Operators fired the RS-25 engine on the Fred Haise Test Stand for almost eight-and-a-half minutes (500 seconds) – the same amount of time needed to help launch SLS – and at power levels ranging between 80% to 113%. New RS-25 engines will power up to the 111% level to provide additional thrust for launch of SLS. Testing up to the 113% power level provides a margin of operational safety.

Now at the halfway point in the series, teams will install a new certification nozzle on the engine. Installation of the new nozzle will allow engineers to gather additional performance data from a second production unit. Following installation next month, testing will resume at Stennis with six additional hot fires scheduled through March.

RS-25 engine with second production nozzle installed
Having reached the halfway point in a 12-test RS-25 certification series, teams at NASA’s Stennis Space Center will install a second production nozzle on the engine to gather additional performance data during the remaining scheduled hot fires.
Aerojet Rocketdyne

For each Artemis mission, four RS-25 engines, along with a pair of solid rocket boosters, power the SLS to produce more than 8.8 million pounds of thrust at liftoff. Under NASA’s Artemis campaign, the agency will establish the foundation for long-term scientific exploration at the Moon, land the first woman, first person of color, and its first international partner astronaut on the lunar surface, and prepare for human expeditions to Mars for the benefit of all.

NASA’s Marshall Space Flight Center manages the SLS Program.

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Cygnus Lifts Off Atop SpaceX Rocket to Deliver Station Cargo

A fresh supply of more than 8,200 pounds of scientific investigations and cargo is on its way to the International Space Station on a Northrop Grumman Cygnus resupply spacecraft after launching on a SpaceX Falcon 9 rocket at 11:07 a.m. CST Jan. 30 from Space Launch Complex 40 at Cape Canaveral Space Force Station.

The Cygnus cargo craft from Northrop Grumman launches atop the SpaceX Falcon 9 rocket at Space Launch Complex 40 at Cape Canaveral Space Force Station on Jan. 30.
The Cygnus cargo craft from Northrop Grumman launches atop the SpaceX Falcon 9 rocket at Space Launch Complex 40 at Cape Canaveral Space Force Station on Jan. 30.
NASA TV

Cygnus has successfully deployed its two solar arrays and is scheduled to arrive at the space station around 3:15 a.m. Feb. 1. NASA+, NASA Television, the NASA app, and agency’s website will provide live coverage of the spacecraft’s approach and arrival beginning at 1:45 a.m.

NASA astronaut Jasmin Moghbeli will capture Cygnus using the station’s Canadarm2 robotic arm, and NASA astronaut Loral O’Hara will be acting as a backup. After capture, the spacecraft will be installed on the Unity module’s Earth-facing port.

This is Northrop Grumman’s 20th contracted resupply mission for NASA.

The Payload Operations Integration Center at NASA’s Marshall Space Flight Center operates, plans, and coordinates the science experiments onboard the space station 365 days a year, 24 hours a day.

Learn more about station activities by following the space station blog.

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NASA Space Tech Spinoffs Benefit Earth Medicine, Moon to Mars Tools

As NASA innovates for the benefit of all, what the agency develops for exploration has the potential to evolve into other technologies with broader use here on Earth. Many of those examples are highlighted in NASA’s annual Spinoff book including dozens of NASA-enabled medical innovations, as well other advancements.

Inside of an underground subway station, two firefighters carry a robot mounted inside of a trapezoid-shaped wireframe toward a blazing fire. There is a subway car to the firefighters’ right, highlighted by the red, yellow, and orange hue of a fire in the background. The robot helps firefighters and other first responders protect their lives and the lives of others by investigating hazardous situations.
Squishy Robotics’ Tensegrity Sensor Robots help first responders determine their approach to a disaster scene. Firefighters used the robots during a subway attack exercise at the 2021 Unmanned Tactical Application Conference to detect gas leaks and other hazards.
Credits: FLYMOTION LLC.

This year’s publication, NASA’s 2024 Spinoff, features several commercialized technologies using the agency’s research and development expertise to impact everyday lives, including:

“As we continue to push new frontiers and do the unimaginable, NASA’s scientists and engineers are constantly innovating and advancing technologies,” said NASA Administrator Bill Nelson. “A critical part of our mission is to quickly get those advances into the hands of companies and entrepreneurs who can use them to grow their businesses, open new markets, boost the economy, and raise the quality of life for everyone.”

The medical innovations include the first wireless arthroscope – a small tube carrying a camera inserted into the body during surgery – to receive clearance from the U.S. Food and Drug Administration, which benefited from NASA’s experience with spacesuits and satellite batteries. Technologies for diagnosing illnesses like the coronavirus, hepatitis, and cancer have also stemmed from NASA’s space exploration and science endeavors. Even certain types of toothpaste originated from the agency’s efforts to grow crystals for electronics.

Additional 2024 Spinoff highlights include developments under  NASA’s Artemis campaign, like a small, rugged video camera used to improve aircraft safety and a new method for detecting defects or damage in composite materials. Meanwhile, another Spinoff story details the latest benefits of fuel cell technology created more than 50 years ago for Apollo, which is now poised to support terrestrial power grids based on renewable energy.

The book also features several technologies NASA has identified as promising future spinoffs and information on how to license agency tech. Since the 1970s, thousands of NASA technologies have found their way into many scientific and technical disciplines, impacting nearly every American industry.

“As NASA’s longest continuously running program, we continue to increase the number of technologies we license year-over-year while streamlining the development path from the government to the commercial sector,” said Daniel Lockney, Technology Transfer program executive at NASA Headquarters. “These commercialization success stories continually prove the benefits of transitioning agency technologies into private hands, where the real impacts are made.”

Spinoffs are part of NASA’s Space Technology Mission Directorate and its Technology Transfer program. Tech Transfer is charged with finding broad, innovative applications for NASA-developed technology through partnerships and licensing agreements, ensuring agency investments benefit the nation and the world.

Read the latest issue of Spinoff.

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Webb Depicts Staggering Structure in 19 Nearby Spiral Galaxies

It’s oh-so-easy to be absolutely mesmerized by these spiral galaxies. Follow their clearly defined arms, which are brimming with stars, to their centers, where there may be old star clusters and – sometimes – active supermassive black holes. Only NASA’s James Webb Space Telescope can deliver highly detailed scenes of nearby galaxies in a combination of near- and mid-infrared light – and a set of these images was publicly released Jan. 29.

These Webb images are part of a large, long-standing project, the Physics at High Angular resolution in Nearby GalaxieS, or PHANGS, program, which is supported by more than 150 astronomers worldwide. Before Webb took these images, PHANGS was already brimming with data from NASA’s Hubble Space Telescope, the Very Large Telescope’s Multi-Unit Spectroscopic Explorer, and the Atacama Large Millimeter/submillimeter Array. These included observations in ultraviolet, visible, and radio light. Webb’s near- and mid-infrared contributions have provided several new puzzle pieces.

The James Webb Space Telescope observed 19 nearby face-on spiral galaxies in near- and mid-infrared light as part of its contributions to the Physics at High Angular resolution in Nearby GalaxieS, or PHANGS, program. PHANGS also includes images and data from NASA’s Hubble Space Telescope, the Very Large Telescope’s Multi-Unit Spectroscopic Explorer, and the Atacama Large Millimeter/submillimeter Array, which included observations taken in ultraviolet, visible, and radio light.
The James Webb Space Telescope observed 19 nearby face-on spiral galaxies in near- and mid-infrared light as part of its contributions to the Physics at High Angular resolution in Nearby GalaxieS, or PHANGS, program. PHANGS also includes images and data from NASA’s Hubble Space Telescope, the Very Large Telescope’s Multi-Unit Spectroscopic Explorer, and the Atacama Large Millimeter/submillimeter Array, which included observations taken in ultraviolet, visible, and radio light.
NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), PHANGS Team, Elizabeth Wheatley (STScI))

“Webb’s new images are extraordinary,” said Janice Lee, a project scientist for strategic initiatives at the Space Telescope Science Institute in Baltimore. “They’re mind-blowing even for researchers who have studied these same galaxies for decades. Bubbles and filaments are resolved down to the smallest scales ever observed, and tell a story about the star formation cycle.”

Excitement rapidly spread throughout the team as the Webb images flooded in. “I feel like our team lives in a constant state of being overwhelmed – in a positive way – by the amount of detail in these images,” added Thomas Williams, a postdoctoral researcher at the University of Oxford in the United Kingdom.

Webb’s NIRCam (Near-Infrared Camera) captured millions of stars in these images, which sparkle in blue tones. Some stars are spread throughout the spiral arms, but others are clumped tightly together in star clusters.

Face-on spiral galaxy, NGC 628, is split diagonally in this image: The James Webb Space Telescope’s observations appear at top left, and the Hubble Space Telescope’s on bottom right. Webb and Hubble’s images show a striking contrast, an inverse of darkness and light. Why? Webb’s observations combine near- and mid-infrared light and Hubble’s showcase visible light. Dust absorbs ultraviolet and visible light, and then re-emits it in the infrared. In Webb's images, we see dust glowing in infrared light. In Hubble’s images, dark regions are where starlight is absorbed by dust.
Face-on spiral galaxy, NGC 628, is split diagonally in this image: The James Webb Space Telescope’s observations appear at top left, and the Hubble Space Telescope’s on bottom right. Webb and Hubble’s images show a striking contrast, an inverse of darkness and light. Why? Webb’s observations combine near- and mid-infrared light and Hubble’s showcase visible light. Dust absorbs ultraviolet and visible light, and then re-emits it in the infrared. In Webb’s images, we see dust glowing in infrared light. In Hubble’s images, dark regions are where starlight is absorbed by dust.
NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), and the PHANGS team

The telescope’s MIRI (Mid-Infrared Instrument) data highlights glowing dust, showing us where it exists around and between stars. It also spotlights stars that haven’t yet fully formed – they are still encased in the gas and dust that feed their growth, like bright red seeds at the tips of dusty peaks. “These are where we can find the newest, most massive stars in the galaxies,” said Erik Rosolowsky, a professor of physics at the University of Alberta in Edmonton, Canada.

Something else that amazed astronomers? Webb’s images show large, spherical shells in the gas and dust. “These holes may have been created by one or more stars that exploded, carving out giant holes in the interstellar material,” explained Adam Leroy, a professor of astronomy at the Ohio State University in Columbus.

Now, trace the spiral arms to find extended regions of gas that appear red and orange. “These structures tend to follow the same pattern in certain parts of the galaxies,” Rosolowsky added. “We think of these like waves, and their spacing tells us a lot about how a galaxy distributes its gas and dust.” Study of these structures will provide key insights about how galaxies build, maintain, and shut off star formation.

Webb Telescope’s view face-on of spiral galaxy NGC 4254.
Webb Telescope’s view face-on of spiral galaxy NGC 4254.
NASA, ESA, CSA, STScI, Janice Lee (STScI), Thomas Williams (Oxford), and the PHANGS team

Evidence shows that galaxies grow from inside out – star formation begins at galaxies’ cores and spreads along their arms, spiraling away from the center. The farther a star is from the galaxy’s core, the more likely it is to be younger. In contrast, the areas near the cores that look lit by a blue spotlight are populations of older stars.

What about galaxy cores that are awash in pink-and-red diffraction spikes? “That’s a clear sign that there may be an active supermassive black hole,” said Eva Schinnerer, a staff scientist at the Max Planck Institute for Astronomy in Heidelberg, Germany. “Or, the star clusters toward the center are so bright that they have saturated that area of the image.”

There are many avenues of research that scientists can begin to pursue with the combined PHANGS data, but the unprecedented number of stars Webb resolved are a great place to begin. “Stars can live for billions or trillions of years,” Leroy said. “By precisely cataloging all types of stars, we can build a more reliable, holistic view of their life cycles.”

In addition to immediately releasing these images, the PHANGS team has also released the largest catalog to date of roughly 100,000 star clusters. “The amount of analysis that can be done with these images is vastly larger than anything our team could possibly handle,” Rosolowsky emphasized. “We’re excited to support the community so all researchers can contribute.”

See the full set of 19 images from both Webb and Hubble.

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 the Canadian Space Agency. Several NASA centers contributed to the project, including NASA’s Marshall Space Flight Center.

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Poised for Science: NASA’s Europa Clipper Instruments are All Aboard

With less than nine months remaining in the countdown to launch, NASA’s Europa Clipper mission has passed a major milestone: Its science instruments have been added to the massive spacecraft, which is being assembled at the agency’s JPL (Jet Propulsion Laboratory).

Set to launch from NASA’s Kennedy Space Center in October, the spacecraft will head to Jupiter’s ice-encased moon Europa, where a salty ocean beneath the frozen surface may hold conditions suitable for life. Europa Clipper won’t be landing; rather, after arriving at the Jupiter system in 2030, the spacecraft will orbit Jupiter for four years, performing 49 flybys of Europa and using its powerful suite of nine science instruments to investigate the moon’s potential as a habitable environment.

NASA’s Europa Clipper, with all of its instruments installed, is visible in the clean room of High Bay 1 at the agency’s Jet Propulsion Laboratory on Jan. 19. The tent around the spacecraft was erected to support electromagnetic testing.
NASA’s Europa Clipper, with all of its instruments installed, is visible Jan. 19 in the clean room of High Bay 1 at the agency’s Jet Propulsion Laboratory. The tent around the spacecraft was erected to support electromagnetic testing.
NASA/JPL-Caltech

“The instruments work together hand in hand to answer our most pressing questions about Europa,” said JPL’s Robert Pappalardo, the mission’s project scientist. “We will learn what makes Europa tick, from its core and rocky interior to its ocean and ice shell to its very thin atmosphere and the surrounding space environment.”

The hallmark of Europa Clipper’s science investigation is how all of the instruments will work in sync while collecting data to accomplish the mission’s science objectives. During each flyby, the fully array of instruments will gather measurements and images that will be layered together to paint the full picture of Europa.

“The science is better if we obtain the observations at the same time,” Pappalardo said. “What we’re striving for is integration, so that at any point we are using all the instruments to study Europa at once and there is no need to have to trade off among them.”

By studying the environment around Europa, scientists will learn more about the moon’s interior. The spacecraft carries a magnetometer to measure the magnetic field around the moon. That data will be key to understanding the ocean, because the field is created, or induced, by the electrical conductivity of the ocean’s saltwater as Europa moves through Jupiter’s strong magnetic field. Working in tandem with the magnetometer is an instrument that will analyze the plasma (charged particles) around Europa, which can distort magnetic fields. Together, they’ll ensure the most accurate measurements possible.

What the mission discovers about Europa’s atmosphere will also lend insights into the moon’s surface and interior. While the atmosphere is faint, with only 100 billionth the pressure of Earth’s atmosphere, scientists expect that it holds a trove of clues about the moon. They have evidence from space- and ground-based telescopes that there may be plumes of water vapor venting from beneath the moon’s surface, and observations from past missions suggest that ice and dust particles are being ejected into space by micrometeorite impacts.

Three instruments will help investigate the atmosphere and its associated particles: A mass spectrometer will analyze gases, a surface dust analyzer will examine dust, and a spectrograph will collect ultraviolet light to search for plumes and identify how the properties of the dynamic atmosphere change over time.

Jupiter’s icy moon Europa holds a vast internal ocean that could have conditions suitable for life. NASA’s Europa Clipper mission will help scientists better understand the potential for habitable worlds beyond our planet. (NASA/JPL-Caltech)

All the while, Europa Clipper’s cameras will be taking wide- and narrow-angle pictures of the surface, providing the first high-resolution global map of Europa. Stereoscopic, color images will reveal any changes in the surface from geologic activity. A separate imager that measures temperatures will help scientists identify warmer regions where water or recent ice deposits may be near the surface.

An imaging spectrometer will map the ices, salts, and organic molecules on the moon’s surface. The sophisticated set of imagers will also support the full instrument suite by collecting visuals that will provide context for the set of data collected.

Of course, scientists also need a better understanding of the ice shell itself. Estimated to be about 10 to 15 miles thick, this outer casing may be geologically active, which could result in the fracture patterns that are visible at the surface. Using the radar instrument, the mission will study the ice shell, including searching for water within and beneath it. (The instrument’s electronics are now aboard the spacecraft, while its antennas will be mounted to the spacecraft’s solar arrays at Kennedy later this year.)

Finally, there’s Europa’s interior structure. To learn more about it, scientists will measure the moon’s gravitational field at various points in its orbit around Jupiter. Observing how signals transmitted from the spacecraft are tugged on by Europa’s gravity can tell the team more about the moon’s interior. Scientists will use the spacecraft’s telecommunications equipment for this science investigation.

With all nine instruments and the telecommunications system aboard the spacecraft, the mission team has begun testing the complete spacecraft for the first time. Once Europa Clipper is fully tested, the team will ship the craft to Kennedy in preparation for launch on a SpaceX Falcon Heavy rocket.

Europa Clipper’s main science goal is to determine whether there are places below Jupiter’s icy moon, Europa, that could support life. The mission’s three main science objectives are to determine the thickness of the moon’s icy shell and its surface interactions with the ocean below, to investigate its composition, and to characterize its geology. The mission’s detailed exploration of Europa will help scientists better understand the astrobiological potential for habitable worlds beyond our planet.

Managed by Caltech in Pasadena, California, NASA’s JPL leads the development of the Europa Clipper mission in partnership with the Johns Hopkins Applied Physics Laboratory (APL) in Laurel, Maryland, for NASA’s Science Mission Directorate. APL designed the main spacecraft body in collaboration with JPL and NASA’s Goddard Space Flight Center. The Planetary Missions Program Office at NASA’s Marshall Space Flight Center executes program management of the Europa Clipper mission.

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Hubble Observes a Galactic Distortion

The galaxy NGC 5427 shines in a new NASA Hubble Space Telescope image. It’s part of the galaxy pair Arp 271, and its companion NGC 5426 is located below this galaxy and outside of this image’s frame. However, the effects of the pair’s gravitational attraction is visible in the galactic distortion and cosmic bridge of stars seen in the lower-right region of the image.

Hubble Observes a Galactic Distortion
The galaxy NGC 5427 shines in this new NASA Hubble Space Telescope image.
NASA, ESA, and R. Foley (University of California – Santa Cruz); Processing: Gladys Kober (NASA/Catholic University of America

In 1785, British astronomer William Herschel discovered the pair, which is locked in an interaction that will last for tens of millions of years. Whether they will ultimately collide and merge is still uncertain, but their mutual gravitational attraction has already birthed many new stars. These young stars are visible in the faint bridge connecting the two galaxies, located at the bottom of the image. Such a bridge provides an avenue for the two galaxies to continue sharing the gas and dust that becomes new stars.

Hubble Observes a Galactic Distortion
The galaxy NGC 5427 shines in the large image from Hubble, with ground-based observations showing its companion galaxy NGC 5426. Together, this pair is known as Arp 271.
NASA, ESA, and R. Foley (University of California – Santa Cruz); Processing: Gladys Kober (NASA/Catholic University of America

Scientists believe Arp 271 can serve as a blueprint for future interactions between our Milky Way Galaxy and our neighbor the Andromeda Galaxy, expected to happen in about 4 billion years.

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      Explore This Section Earth Home Earth Observer Home Editor’s Corner Feature Articles Meeting Summaries News Science in the News Calendars In Memoriam More Archives 8 min read
      AGU 2024: NASA Science on Display in the Nation’s Capital
      Introduction
      The American Geophysical Union (AGU) returned to the nation’s capital in 2024, hosting its annual meeting at the Walter E. Washington Convention Center in Washington, DC from December 9–14, 2024. NASA Science upheld its long-standing tradition as an AGU partner and exhibitor, leveraging the meeting as an opportunity to share NASA’s cutting-edge research, data, and technology with the largest collection of Earth and planetary science professionals in the world. Many of the estimated 25,000 students, scientists, and industry personnel who attended the conference visited the NASA Science exhibit, interacting with NASA subject matter experts as detailed in the essay that follows – see Photo 1. Visitors also watched live Hyperwall presentations and collected NASA Science outreach materials, such as the 2025 NASA Science Planning Guide.
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      NASA Hyperwall Stories
      The NASA Hyperwall has been a focal point of the agency’s outreach efforts for over two decades, serving as both a powerful storytelling platform and the primary vehicle through which the public engages with the award-winning visualizations published by NASA’s Scientific Visualization Studio (SVS) – see Photo 2. Forty-nine NASA mission scientists and program representatives shared NASA science with the public from the Hyperwall stage during AGU24. NASA leadership shared mission news and outlined upcoming research across all five of the NASA Science divisions: Earth science, planetary science, heliophysics, astrophysics, and biological and physical sciences – see Photos 3–8. A catalog of NASA project scientists and mission representatives, who provided colorful overviews of everything from NASA’s Mars Sample Return to the Parker Solar Probe’s historic flyby of the Sun, delivered additional presentations. 
      Photo 2. Mark Subbarao [NASA GSFC—Director of NASA’s Scientific Visualization Studio] highlighted key visualizations produced by NASA’s Scientific Visualization Studio during 2024 and presented them as a countdown of the top 10 visualizations of the year. Photo credit: NASA The complete AGU24 Hyperwall schedule is available at this link. Readers can view YouTube videos of the presentations via links over the individual names in the photo captions below.
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      Photo 9a. In partnership with AGU, student winners of the 2024 AGU Michael Freilich Student Visualization Competition received prizes and presented their work at the NASA hyperwall stage. Steve Platnick [NASA GSFC—Research Scientist for Earth Science Division ] [left with back to camera] congratulates Caitlin Haedrich [NC State University—Ph.D. candidate, contest winner (CW)]. Photo credit: NASA Photo 9b. Standing on the NASA Hyperwall stage [left to right] are Erik Hankin [AGU—Assistant Director of Career and Student Programs], Barry Lefer [NASA HQ—Program Manager for the Tropospheric Composition Program (TCP)], Mya Thomas [University of Missouri-Kansas City—Undergraduate Student.  CW], Mariliee Karinshak [Washington University in St. Louis—Undergraduate Student, CW], Swati Singh [Auburn University—PhD Candidate, CW], Crisel Suarez [Vanderbilt University—PhD Candidate, CW], and Steve Graham [GSFC/Global Science & Technology Inc.—NASA Science Support Office Task Leader]. Photo credit: NASA Photo 9c. Patrick Kerwin [University of Arizona—Graduate Student, CW] delivers his award-winning talk titled Earth Observation for Disaster Response: Highlighting Applied Products. Photo credit: NASA




      Face-to-face With NASA Experts
      AGU opened its exhibit hall to the public at 10:00 AM on December 9. Thousands of eager attendees poured into the space to engage with exhibit staff, representing a variety of universities, research institutions, and private organizations from around the world.
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      NASA Science welcomed AGU attendees, who gathered within the perimeter of the exhibit shortly after opening – see Photo 10 – where NASA staff distributed the 2025 NASA Science Planning Guide – see Photo 11.
      Attendees filtered through the NASA Science booth by the thousands, where more than 130 outreach specialists and subject matter experts from across the agency were available to share mission-specific science and interface directly with members of the public – see Photos 12–15.
      Photo 12. The NASA Science booth included a collection of exhibit tables, where mission scientists and outreach specialists shared information and materials specific to various NASA missions and programs. Photo credit: NASA Photo 13. Outreach specialists from NASA’s Dragonfly mission, which plans to send a robotic aircraft to the surface of Saturn’s moon Titan, speak with attendees in front of a to-scale model of the aircraft. Photo credit: NASA Photo 14. Staff from NASA’s astrobiology program share a collection of graphic novels produced by graphic artist Aaron Gronstal, highlighting the research that the program conducts to answer important questions about the origin, evolution, and distribution of life in the universe. Photo credit: NASA Photo 15. Exhibit staff and AGU attendees interact with three-dimensional (3D) models of NASA spacecraft and technology in augmented reality. Photo credit: NASA AGU attendees met with project scientists and experts at a new exhibit, called “Ask Me Anything.” The discussions spanned a variety of NASA missions, including Mars Sample Return, James Webb Space Telescope, and Parker Solar Probe, with specialists from these and other missions who spoke during the sessions – see Photo 16. An installation of NASA’s Earth Information Center also made an appearance at AGU24, providing attendees with additional opportunities to speak with Earth scientists and learn more about NASA research – see Photo 17.
      Photo 16. NASA Heliophysicists discuss solar science with AGU attendees at the “Ask Me About Heliophysics” table. Photo credit: NASA Photo 17. At the Earth Information Center, attendees spoke with NASA staff about the various ways that NASA keeps tabs on the health of Earth’s atmosphere, oceans, and landmasses from space. Photo credit: NASA 2024 SMD Strategic Content and Integration Meeting
      As they have done for many years now, staff and leadership from NASA’s Science Mission Directorate (SMD) Engagement Branch convened in Washington, DC on December 8 (the day before the Fall AGU meeting began) to discuss agency communications and outreach priorities. This annual meeting provided personnel from each of SMD’s scientific divisions a valuable opportunity to highlight productive strategies and initiatives from the previous calendar year and chart a path for the year ahead. During the single-day event, team leaders shared information related to NASA’s web-modernization efforts, digital outreach strategies, and exhibit presence. Approximately 150 in-person and 50 online NASA staff joined the hybrid meeting.
      After a welcome from Steve Graham [GSFC/GST—NASA Science Support Office Task Leader], who covered meeting logistics, the participants heard from NASA Headquarters’ SMD Engagement and Communication representatives throughout the day. 
      Amy Kaminski [Engagement Branch Chief], who recently replaced Kristen Erickson in this role, used this opportunity to more formally introduce herself to those who might not know her and share her visions for engagement. Karen Fox [Senior Science Communications Official] discussed the evolution of communication for SMD missions over the past decade – moving from siloed communications a decade ago that very much focused on “my mission,” to a much more cooperation between missions and focus on thematic communications. Following up on Kaminski’s remarks that gave an overall vision for engagement, and Fox’s remarks about how having a vision will help streamline our messaging, Alex Lockwood [Strategic Messaging and Engagement Lead] delved into the nuts and bolts of strategic planning, with focus on the use of work packages and memorandums of understanding for promoting upcoming missions.
      After the leadership set the tone for the meeting, Emily Furfaro [NASA Science Digital Manager] gave a rapid tour of many of NASA’s digital assets intended to give participants an idea of the vast resources available for use. Diana Logreira [NASA Science Public Web Manager] then laid out some principles to be followed in developing unified vision for the NASA Science public web experience.
      In the afternoon, there were individual breakout sessions for the Earth Science, Planetary Science, and Heliophysics divisions. These sub-meetings were led by Ellen Gray, Erin Mahoney, and Deb Hernandez, Engagement Leads for Earth Science, Heliophysics, and Planetary Sciences respectively.  These breakout sessions afforded participants with an opportunity to focus on ideas and goals specific to their own divisions for 2025. In the Earth Science breakout session, participants heard from other several other speakers who discussed the beats, or content focus areas, that had been chosen for Earth Science Communications in 2024 – including oceans and Earth Action (formerly known as Applied Sciences) – and those that have been identified for 2025: technology, land science, and continued focus on Earth Action.
      Photo 18a. NASA Science Mission Directorate staff gathers in Washington, DC ahead of AGU for the annual meeting, where in-person attendees hear from leadership and work collaboratively to refine communications strategies for 2025.  Photo credit: NASA Photo 18b. Joseph Westlake [NASA HQ—Heliophysics Division Director] discusses division-specific goals with Heliophysics communication leads during the division’s “breakout session.” Photo credit: NASA Photo 18c. Science Mission Directorate leadership fields questions from SMD staff during the end-of-meeting panel discussion. Photo credit: NASA




      After participants reconvened from the breakouts, Nicola Fox [Associate Administrator, Science Mission Directorate] gave a mid-afternoon presentation in which she presented her perspective on integrated NASA science, which led into a one-hour “Ask Us” panel with Division Directors to conclude the meeting. Participants included: Mark Clampin [Astrophysics], Lisa Carnell [Biological], Julie Robinson [Earth Science, Deputy], Joe Westlake [Heliophysics], John Gagosian [Joint Agency Satellite], Charles Webb [Planetary Science, Acting].
      Based on this meeting, and other communications guidance from NASA HQ, a few general SMD/Earth Science content and engagement priorities for 2025 have emerged. They include:
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      The NASA exhibit is an important component of the agency’s presence at AGU, and NASA leverages its large cohort of scientists who participate in the exchange of information and ideas outside of the exhibit hall – in plenary meetings, workshops, poster sessions, panels, and informal discussions. AGU sessions and events that featured NASA resources, scientists, and program directors included the Living with a Star Town Hall, NASA’s Early Career Research Program, NASA’s Sea Level Change Team: Turning Research into Action, and many more. Click here for the complete list of NASA-related events at AGU24.
      As the final event in a busy calendar of annual scientific conferences, AGU is often an opportunity for NASA scientists to publish findings from the previous year and set goals for the year ahead. Just as they did in 2024, the agency’s robust portfolio of missions and programs will continue to set new records, such as NASA’s Parker Solar Probe pass of the Sun, and conduct fundamental research in the fields of Earth and space science.
      The 2025 AGU annual meeting will be held at the New Orleans Ernest N. Morial Convention Center, in New Orleans, LA, from December 15–19, 2025. See you there.
      Nathan Marder
      NASA’s Goddard Space Flight Center/Global Science & Technology Inc.
      nathan.marder@nasa.gov
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      6 Min Read NASA Marshall Reflects on 65 Years of Ingenuity, Teamwork 
      NASA’s Marshall Space Flight Center in Huntsville, Alabama, is celebrating its 65-year legacy of ingenuity and service to the U.S. space program – and the expansion of its science, engineering, propulsion, and human spaceflight portfolio with each new decade since the NASA field center opened its doors on July 1, 1960.
      What many Americans likely call to mind are the “days of smoke and fire,” said Marshall Director Joseph Pelfrey, referring to the work conducted at Marshall to enable NASA’s launch of the first Mercury-Redstone rocket and the Saturn V which lifted Americans to the Moon, the inaugural space shuttle mission, and the shuttle flights that carried the Hubble Space Telescope, Chandra X-ray Observatory, and elements of the International Space Station to orbit. Most recently, he said they’re likely to recall the thunder of NASA’s SLS (Space Launch System), rising into the sky during Artemis I.
      NASA’s Space Launch System, carrying the Orion spacecraft, launches on the Artemis I flight test on Nov. 16, 2022. NASA’s Marshall Space Flight Center in Huntsville, Alabama, led development and oversees all work on the new flagship rocket, building on its storied history of propulsion and launch vehicle design dating back to the Redstone and Saturn rockets. The most powerful rocket ever built, SLS is the backbone of NASA’s Artemis program, set to carry explorers back to the Moon in 2026, help establish a permanent outpost there, and make possible new, crewed journeys to Mars in the years to come.NASA/Bill Ingalls Yet all the other days are equally meaningful, Pelfrey said, highlighting a steady stream of milestones reflecting the work of Marshall civil service employees, contractors, and industry partners through the years – as celebrated in a new “65 Years of Marshall” timeline.
      “The total sum of hours, contributed by tens of thousands of men and women across Marshall’s history, is incalculable,” Pelfrey said. “Together they’ve blended legacy with innovation – advancing space exploration and scientific discovery through collaboration, engineering excellence, and technical solutions. They’ve invented and refined technologies that make it possible to safely live and work in space, to explore other worlds, and to help safeguard our own.
      The total sum of hours, contributed by tens of thousands of men and women across Marshall’s history, is incalculable.
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      “Days of smoke and fire may be the most visible signs, but it’s the months and years of preparation and the weeks of post-launch scientific discovery that mark the true dedication, sacrifice, and monumental achievements of this team.”
      Reflecting on Marshall history
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      “Test, retest, and then fly – that’s what we did here at the start,” said retired engineer Harry Craft, who was part of the original U.S. Army rocket development team that moved from Fort Bliss, Texas, to Huntsville to begin NASA’s work at Marshall. “And we did it all without benefit of computers, working out the math with slide rules and pads of paper.”
      The 138-foot-long first stage of the Saturn V rocket is lowered to the ground following a successful static test firing in fall 1966 at the S-1C test stand at NASA’s Marshall Space Flight Center in Huntsville, Alabama. The Saturn V, developed and managed at Marshall, was a multi-stage, multi-engine launch vehicle that stood taller than the Statue of Liberty and lofted the first Americans to the Moon. Its success helped position Marshall as an aerospace leader in propulsion, space systems, and launch vehicle development.NASA “Those were exciting times,” retired test engineer Parker Counts agreed. He joined Marshall in 1963 to conduct testing of the fully assembled and integrated Saturn first stages. It wasn’t uncommon for work weeks to last 10 hours a day, plus weekend shifts when deadlines were looming. 
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      This photograph shows the liquid hydrogen tank and liquid oxygen tank for the Space Shuttle external tank (ET) being assembled in the weld assembly area of the Michoud Assembly Facility (MAF). The ET provides liquid hydrogen and liquid oxygen to the Shuttle’s three main engines during the first eight 8.5 minutes of flight. At 154-feet long and more than 27-feet in diameter, the ET is the largest component of the Space Shuttle, the structural backbone of the entire Shuttle system, and the only part of the vehicle that is not reusable. The ET is manufactured at the Michoud Assembly Facility near New Orleans, Louisiana, by the Martin Marietta Corporation under management of the Marshall Space Flight Center.NASA “We didn’t have cellphones or telecon capabilities yet,” Odom recalled. “I probably spent more time with the pilot of the twin-engine plane in those days than I did with my wife.”
      Marshall’s shuttle propulsion leadership led to the successful STS-1 mission in 1981, launching an era of orbital science exemplified by NASA’s Spacelab program. 
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      Engineers in the X-ray Calibration Facility at NASA’s Marshall Space Flight Center in Huntsville, Alabama, work to integrate elements of the Chandra X-ray Observatory in this March 1997 photo. Chandra was lifted to orbit by space shuttle Columbia on July 23, 1999, the culmination of two decades of telescope optics, mirror, and spacecraft development and testing at Marshall. In the quarter century since, Chandra has delivered nearly 25,000 detailed observations of neutron stars, supernova remnants, black holes, and other high-energy objects, some as far as 13 billion light-years distant. Marshall continues to manage the program for NASA. NASA Bookended by the successful Hubble and Chandra launches, the 1990s also saw Marshall deliver the first U.S. module for the International Space Station, signaling a transformative new era of human spaceflight.
      Odom, who retired in 1989 as associate administrator for the space station at NASA Headquarters, reflects on his three-decade agency career with pride. 
      “It was a great experience, start to finish, working with the teams in Huntsville and New Orleans and our partners nationwide and around the globe, meeting each new challenge, solving the practical, day-to-day engineering and technology problems we only studied about in college,” he said. 
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      As the 2020s continue, Marshall meets each new challenge with enthusiasm and expertise, preparing for the highly anticipated Artemis II crewed launch and a host of new science and discovery missions – and buoyed by strong industry partners and by the Huntsville community, which takes pride in being home to “Rocket City USA.”
      “Humanity is on an upward, outward trajectory,” Pelfrey said. “And day after day, year after year, Marshall is setting the course to explore beyond tomorrow’s horizon.”
      Read more about Marshall and its 65-year history:
      https://www.nasa.gov/marshall
      Hannah Maginot
      Marshall Space Flight Center, Huntsville, Ala.
      256-544-0034
      hannah.l.maginot@nasa.gov  
      Share
      Details
      Last Updated Feb 24, 2025 EditorBeth RidgewayLocationMarshall Space Flight Center Related Terms
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