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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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      Biodiverse regions across California remain vulnerable to harmful wildfires year round. Quantifying and measuring these regions’ wildfire resilience is necessary for understanding where/how to allocate environmental resources. Several ecological wildfire studies have been conducted utilizing artificial intelligence and remote sensing to analyze and predict biodiversity damage across wildfire prone regions, including Northern Algeria and Arkansas, USA. The current case study aims to analyze biodiversity damage from the 2023 Csarf Smith River Complex Fire in Six Rivers National Forest, California and predict the difference in Normalized Burn Ratio (dNBR) and difference in Normalized Difference Vegetation Index (dNDVI) for 2025 and 2028 using remote-sensing-based random forest (RF) regression. Furthermore, to observe, holistically, a practical method California has implemented to address state-wide wildfire damage, the 2019 California Wildfire Fund (AB 1054 and AB 111) was evaluated using the synthetic control method (SCM). For this case study, remote sensing data from the United States Geological Survey (USGS) and NASA (Landsat 9 Satellite C2 L2, TerraClimate and the Land Data Assimilation System) were utilized for processing relevant spectral indexes for the RF. Data from NOAA, Energy Information Agency, International Monetary Fund and Bureau of Economic Analysis were utilized as synthetic control datasets to evaluate the effects of the 2019 California Wildfire Fund. Elevated topography in this study area is susceptible to high severity burn effects, while less elevated topography burns less. This result affected dNBR and dNDVI predictions as elevated areas seemingly did not have strong resilience to rampant burns. This demonstrates a direct correlation to potential lower transpiration rates for elevated areas, warranting further analysis. Results of low variance, post-treatment, between the treated unit and the synthetic control unit, poses concern for the positive effect of the 2019 Wildfire Fund.

      Carrie Hashimoto
      Describing changes in evapotranspiration following the 2020 Creek Fire in the southern Sierra Nevada
      Carrie Hashimoto
      Climatic warming and high tree density have caused larger and more severe wildfires to occur in western United States forests over time. Wildfires affect both the hydrology and ecology of forests via alterations to the water balance (e.g., evapotranspiration, streamflow, infiltration, and more) and could shift vegetation communities and subsequent ecosystem structure and function. This project explores ecological characteristics of a landscape that predict the extent to which the Creek Fire in the southern Sierra Nevada has affected evapotranspiration. Strides in understanding of consequential evapotranspiration changes can create pathways to address emerging forest health challenges posed by similar western fires. For analysis, various remote sensing and modeled data were collected from OpenET, the North American Land Data Assimilation System, TerraClimate, Harmonized LandSat Sentinel-2 data, and the Shuttle Radar Topography Mission. Multiple linear regression and generalized additive models were constructed. Relative change in evapotranspiration served as the response variable. Model covariates included average temperature, total precipitation in the preceding months, average soil moisture, elevation, slope, aspect, northness, latitude, pre-fire normalized difference vegetation index (NDVI), and post-fire change in normalized burn ratio (dNBR). Best subset selection with cross validation demonstrated minimization of cross-validation error with a 7-covariate model. This reduced model yields lower complexity and more interpretability while sustaining an adjusted R2 of 0.626, compared to the full model’s adjusted R2 of 0.663. A reduced generalized additive model (GAM) with interaction terms drawn from the linear model variable selection demonstrated an adjusted R2 of 0.695, indicating a better fit that comes at the cost of reduced interpretability and higher computational requirements than the linear models. The goal of this work is to disentangle environmental indicators of post-fire evapotranspiration change, such that predictive modeling of future wildfire impacts on evapotranspiration can be achieved.


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      Last Updated Nov 22, 2024 Related Terms
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      8 min read SARP East 2024 Ocean Remote Sensing Group
      Article 21 mins ago 10 min read SARP East 2024 Atmospheric Science Group
      Article 21 mins ago 11 min read SARP East 2024 Terrestrial Fluxes Group
      Article 22 mins ago View the full article
    • By NASA
      11 min read
      Preparations for Next Moonwalk Simulations Underway (and Underwater)
      Return to 2024 SARP Closeout Faculty Advisors:
      Dr. Lisa Haber, Virginia Commonwealth University
      Dr. Brandon Alveshere, Virginia Commonwealth University
      Dr. Chris Gough, Virginia Commonwealth University
      Graduate Mentor:
      Mindy Priddy, Virginia Commonwealth University

      Mindy Priddy, Graduate Mentor
      Mindy Priddy, graduate mentor for the 2024 SARP Terrestrial Fluxes group, provides an introduction for each of the group members and shares behind-the scenes moments from the internship.

      Angelina De La Torre
      Using NDVI as a Proxy for GPP to Predict Carbon Dioxide Fluxes
      Angelina De La Torre
      Climate change, driven primarily by greenhouse gases, poses a threat to the future of our planet. Among these gases is carbon dioxide (CO₂), which has a much longer atmospheric residence time compared to other greenhouse gases. One potential factor in reducing atmospheric CO₂ enrichment is plant productivity. Gross Primary Productivity (GPP) estimates the amount of CO₂ fixed during photosynthesis. The Normalized Difference Vegetation Index (NDVI) provides insight into the health of an ecosystem by measuring the density and greenness of vegetation. Therefore, it can be inferred that there is a relationship between NDVI and GPP, as greener plants are likely more productive. In this study, we used NDVI as a proxy for GPP and analyzed the effect NDVI had on CO₂ fluxes during California’s wet season between January and March 2023 in a restored tidal freshwater wetland. GPP and CO₂ flux data were obtained from the Dutch Slough AmeriFlux tower in Oakley, California. Landsat data were used to calculate the average NDVI. The influence of NDVI on GPP was assessed using linear regression. A second linear regression was then performed using NDVI and CO₂ flux, of which GPP is one component. We anticipate that wetlands with greater vegetation density will have lower CO₂ emissions.

      Because Landsat data scans in 16-day intervals, daily variation in NDVI could not be observed. This translates to a frequency discrepancy between the Landsat and AmeriFlux data, as AmeriFlux towers measure in half-hour intervals. Additionally, the wet season represented was limited by data availability, as the data before 2023 were unavailable. Despite data limitations in this study, the outlined process could be repeated in various wetland and climate classifications for further analysis of a larger sample size. This study could assist in developing strategies to increase CO₂ sequestration in an attempt to slow the effects of climate change.

      Samarth Jayadev
      Using Machine Learning to Assess Relationships between NDVI and Net Carbon Exchange During the COVID-19 Pandemic
      Samarth Jayadev
      Understanding the movement of carbon between Earth’s land surface and atmosphere is essential for ecosystem monitoring, creating climate change mitigation strategies, and assessing the carbon budget on national to global scales. Measures of greenness serve as indicators of processes such as photosynthesis that control carbon exchange and are vital in modeling of carbon fluxes. NASA’s Orbiting Carbon Observatory (OCO-2) provides high quality measurements of column-averaged CO₂ concentrations that can be used to derive net carbon exchange (NCE), a measure of CO₂ flux between terrestrial ecosystems and the atmosphere.
      From OCO-2, NCE data collected at the land nadir, land glint satellite position combined with in situ sampling can provide accurate measurements on a 1°x1° scale suitable for carbon flux characterization across the contiguous United States (CONUS). Normalized difference vegetation index (NDVI), which ranges from -1 to +1, measures the greenness of vegetation, serving as an indicator of plant density and health. This can help to understand ecosystem to carbon-cycle interactions and be leveraged for determining patterns with NCE. We examined the relationship between NDVI and NCE across CONUS during 2020 using Gradient Boosting Decision Trees (GBDT) which specialize in classifying and predicting non-linear relationships. This algorithm takes multiple weak learners (decision trees) and combines their predictions in an iterative ensemble method to improve prediction accuracy. Feature and permutation importance tests found that January and August (trough and peak NDVI, respectively) were the highest weighted predictor variables related to NCE. The dataset was split in a 90% training 10% test ratio across latitude/longitude grid cells to assess and verify model performance. Using the mean squared error loss function and hyperparameters with optimal estimators, tree depth, sample split, and learning rate the algorithm was able to converge the test predictions to match the deviance of the training data. The gradient boosting model can be applied to different months and years of NDVI/NCE to further explore these relationships or a multitude of research questions. Further studies should consider integrating land use and land cover change variables such as bare land and urbanization to improve predictions of NCE.

      Makai Ogoshi
      Deep-learning Derived Spaceborne Canopy Structural Metrics Predict Forest Carbon Fluxes
      Makai Ogoshi
      Terrestrial and airborne lidar data products describing canopy structure are potent predictors of forest carbon fluxes, but whether satellite data products produce similarly robust indicators of canopy structure is not known. The assessment of contemporary spaceborne lidar and other remote sensing data products as predictors of carbon fluxes is crucial to next generation instrument and data product design and large-spatial scale modeling. We investigated relationships between deciduous broadleaf forest canopy structure, derived from deep-learning models created with lidar data from GEDI and optical imagery from Sentinel-2, and forest carbon exchange. These included comparisons to in-situ continuous net ecosystem exchange (NEE), gross primary production (GPP), and net primary production (NPP). We find that the mean  canopy height from the gridded spaceborne product has a strong correlation with forest NPP, similar to prior analysis with ground-based lidar (portable canopy lidar; PCL). For comparison to NPP, heights taken from the gridded spaceborne product were compared by overlapping the product with nine terrestrial forest sites from the National Ecological Observatory Network (NEON). We used standard deviation of canopy height as a measure of canopy structural complexity. Complexity derived from the gridded spaceborne product does not show the same strong correlation with NPP as found when using PCL. Mean annual GPP and NEE across five years were compared to the gridded spaceborne product at six Fluxnet2015-tower sites with continuous, gap-filled carbon flux data. When compared to in-situ flux tower data, neither mean canopy height nor structural complexity strongly correlate to annual NEE or GPP. Primarily, the finding that derived spaceborne products exhibit a strong correlation between forest canopy height and NPP will advance global-scale application of forest-carbon flux predictions. Secondarily, a variety of limitations highlight shortcomings in the current terrestrial flux data network. A small number of available study sites, both spatially and temporally, and lack of resolution in vertical complexity of canopy structure both contribute to uncertainty in assessing the relationships to NEE and GPP.

      Sebastian Reed
      Porewater Methane Concentrations Vary Significantly Across A Freshwater Tidal Wetland
      Sebastian Reed
      Methane is a potent greenhouse gas that is over 80 times more powerful than CO₂ at trapping heat and accounts for an estimated 30% of global temperature rise associated with climate change. The largest natural source of methane worldwide is wetlands. Despite the role of methane in driving climate change, the magnitude of global annual wetland methane flux remains highly uncertain. This study analyzes the effects of greenness (assessed using Normalized Difference Vegetation Index; NDVI), plant species composition, rooting depth, atmospheric methane concentration, and plant longevity on porewater methane concentration at the Kimages Rice Rivers Center tidal freshwater wetland. Samples for atmospheric and porewater concentrations were conducted in situ in June 2024. For each sampling location (n = 23) we collected whole air samples (WAS) 2m above the marsh surface and porewater samples 5cm below the marsh surface. We visually assessed species composition at each sample location, with 12 species of wetland plants present overall. We used the TRY plant database to find the rooting depth, leaf nitrogen content, and lifespan of each species. Drone multispectral data from 2023 was used to estimate NDVI values. These variables were compared to the pore water methane concentration via stepwise linear regression. Leaf N content, NDVI, plant species, and WAS sampling did not show statistically significant correlation to porewater methane concentration. Rooting depth showed a slight positive correlation with porewater methane (alpha = 0.1, p = 0.08, R^2 = 0.1). Samples with only perennial plants (as opposed to annual plants) had a higher mean value of porewater methane (p = 0.1). Analyzing porewater methane provides insight as to what wetland components affect methanogenesis and methane release, which aids in assessing which plant functional traits are most responsible for driving or mitigating climate change. Results from this study and future research in this area has the potential to more accurately assess how methane cycles through wetlands to the atmosphere.

      Nohemi Rodarte
      Understanding the vertical profile of CO₂ concentration: How carbon dioxide levels change with altitude
      Nohemi Rodarte
      Carbon dioxide (CO₂) is one of the main greenhouse gasses that contribute to global warming.While the relationship between CO₂ concentrations and land cover types, such as forests and urban areas, is well documented, there is limited knowledge of how CO₂ concentrations vary with altitude at fine spatial scales. Guided by our hypothesis that CO₂ levels vary with altitude and increase with elevation, we used airborne data collected from the B200 aircraft, which flew at different altitudes (400 to 1200 feet) above the urban area of Hopewell, Virginia, between 9:40 AM and 10:40 AM. We analyzed the CO₂ concentrations recorded by the flight to obtain the median and range for each 100 feet of altitude. Our results reveal that carbon dioxide concentrations varied significantly across the range of altitudes investigated. Within the area studied, CO₂ concentrations were found to range between 410 and 470 ppm. The distribution of these concentrations along the altitude gradient shows a bimodal pattern, with notable peaks at altitudes of 700 to 800 feet and 1100 to 1200 feet. Although CO₂ levels were present at all measured altitudes, there was a noticeable drop in the mean concentration at 800 feet,which then stabilized until reaching 1,000 feet before rising again. This pattern indicates that the concentrations of this greenhouse gas are not uniformly distributed with altitude, but rather vary significantly, showing higher concentrations at certain elevations and lower concentrations at others. The CO₂ distribution fluctuates with altitude, showing higher or lower levels at specific heights rather than a smooth gradient, indicating that altitude impacts CO₂ concentrations. While we did not identify the drivers of this change, future studies could evaluate how factors such as surface emissions, atmospheric mixing, and local conditions may contribute to vertical CO₂ profiles, since the altitudes we considered in this research are within the troposphere.

      Camille Shaw
      Linking NDVI with CO₂ and CH₄ Fluxes: Insights into Vegetation and Urban Source-Sink Dynamics in the Great Dismal Swamp
      Camille Shaw
      In recent years, carbon dioxide, methane, and other greenhouse gases have gained attention because of their contribution to the rise in Earth’s global mean temperature. Methane and carbon dioxide have various sources and sinks, but an expanding array of sources have created a need to assess ongoing change in carbon balance. This study aims to quantify the relationship between Normalized Difference Vegetation Index, or NDVI, and methane and carbon dioxide fluxes. We measured carbon dioxide and methane concentrations within the boundary layer using the PICARRO instrument, focusing on the Great Dismal Swamp, a forested wetland, and surrounding areas in the Eastern Mid-Atlantic Region. Data collection occurred at various times of day and along different flight paths in 2016, 2017, and 2024, with each year representing data from a single season, either spring or fall, for temporal analysis. We calculated methane and carbon dioxide fluxes along the flight paths using airborne eddy covariance, a method for capturing accurate flux measurements while accounting for the mixing of gases in the boundary layer caused by heat. Additionally, we calculated NDVI for this area using NASA’s Landsat 8 and 9 satellite imagery. Analysis of the afternoon flight data revealed a negative linear correlation between NDVI and carbon dioxide flux. Urban areas, characterized by low NDVI, exhibit a positive carbon dioxide flux as a consequence of emissions from vehicles, while forested areas, with high NDVI, show a negative carbon dioxide flux because of photosynthesis. In contrast, methane flux shows minimal correlation with NDVI. The lack of correlation arises because forested wetlands, with high NDVI, emit substantial amounts of methane, while urban areas, despite having low NDVI, still produce significant methane emissions from landfills and industrial activities. Future research could further investigate how seasonal and diurnal variations influence the correlations between NDVI and greenhouse gases by collecting comprehensive data across all seasons within a given year and at various times of the day.

      Return to 2024 SARP Closeout Share
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      Last Updated Nov 22, 2024 Related Terms
      General Explore More
      8 min read SARP East 2024 Ocean Remote Sensing Group
      Article 21 mins ago 10 min read SARP East 2024 Atmospheric Science Group
      Article 21 mins ago 10 min read SARP East 2024 Hydroecology Group
      Article 21 mins ago View the full article
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