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The Marshall Star for October 11, 2023


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The Marshall Star for October 11, 2023

Cyclists compete during the bicycle portion of “Racin’ the Station.”
Cyclists compete during the bicycle portion of “Racin’ the Station.”
Credits: NASA/Mick Speer

Marshall Presents Small Business Awards for 2023

NASA’s Marshall Space Flight Center honored top contractors, subcontractors, teams, and individuals of fiscal year 2023 at the 36th meeting of the Marshall Small Business Alliance.

David Brock, small business specialist at Marshall Space Flight Center, welcomes attendees of the 36th Marshall Small Business Alliance meeting and 17th Industry & Advocate Awards.
David Brock, small business specialist at Marshall Space Flight Center, welcomes attendees of the 36th Marshall Small Business Alliance meeting and 17th Industry & Advocate Awards.
NASA/Mick Speer

The event took place Sept. 21 at the U.S. Space & Rocket Center’s Davidson Center for Space Exploration. Around 600 participants from industry and government gathered to network, learn about business opportunities, and recognize outstanding achievements in support of NASA’s mission and the small business community.

“Marshall is an engine of opportunity for its community and beyond,” said David Brock, small business specialist in Marshall’s Office of Procurement.

Leah Fox, program specilaist for Marshall’s Center Operations talks with an attendee of the 36th Marshall Small Business Alliance Meeting.
Leah Fox, program specilaist for Marshall’s Center Operations talks with an attendee of the 36th Marshall Small Business Alliance Meeting.
NASA/Mick Speer

Marshall’s Industry & Advocate Awards are presented annually and reflect leadership in business community and sustained achievement in service to NASA’s mission.

This year’s award recipients are:

Small Business Prime Contractor of the Year

Victory Solutions Inc.

Small Business Subcontractor of the Year

Waterfront Technical Services

Large Business Prime Contractor of the Year

Jacobs Space Exploration Group

Small Business Mentor-Protégé of the Year Award

Jacobs/CH2M and K.S. Ware

Procurement Person of the Year

Dana Justice, Marshall Office of Procurement

Program Team of the Year

2023 Small Business Action Team, Marshall Office of Procurement

Michelle Anzalone, Ashley Cox, Stephanie Darnell, John David Eagan, Dana Justice, and Josh Wilbourn

Small Business Technical Advisor of the Year

Chip Jones, Marshall Science & Technology Office     

Small Business Technical Person of the Year

Karen Lawler, Marshall Office of the Chief Financial Officer

John Cannaday, director of Marshall’s Office of Procurement, gives opening remarks at the 36th Small Business Alliance Meeting and Industry & Advocacy Awards.
John Cannaday, director of Marshall’s Office of Procurement, gives opening remarks at the 36th Small Business Alliance Meeting and Industry & Advocacy Awards.
NASA/Mick Speer

NASA civil service employees nominate eligible individuals and organizations for awards. A panel of NASA procurement and technical officials evaluates each nominee’s business practices, innovative processes, adoption of new technologies and their overall contributions to NASA’s mission and the agency’s Small Business Program.

Award recipients in the following categories become candidates for agency-level Small Business Industry and Advocate Awards:

  • Large and Small Business Prime Contractors of the Year
  • Small Business Subcontractor of the Year
  • Procurement Team or Person
  • Technical, Small Business Technical Coordinator/Technical Advisor
  • Program Person or Team of the Year

Learn more about Marshall’s small business initiatives.

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NASA Announces Teams for 2024 Student Launch Challenge

NASA has announced the 70 teams representing 24 states and Puerto Rico selected to compete in the 2024 Student Launch Challenge.

The annual competition – one of NASA’s nine Artemis Student Challenges – requires middle/high school and college/university students to design, build, and fly a high-powered amateur rocket and scientific payload.

Students from the AIAA Orange Country Section team of Irvine, California, display their rocket to news media and the public during Rocket Fair – an annual showcase event of NASA’s Student Launch competition April 2023.
Students from the AIAA Orange Country Section team of Irvine, California, display their rocket to news media and the public during Rocket Fair – an annual showcase event of NASA’s Student Launch competition April 2023.
NASA

The nine-month-long challenge will culminate with on-site events April 10-14, 2024, with final launches April 13 at Bragg Farms in Toney, Alabama, just minutes north of NASA’s Marshall Space Flight Center. Teams are not required to travel for their final launch, having the option to launch from a qualified. Details are outlined in the Student Launch Handbook.

Each year NASA implements a new payload challenge to reflect relevant missions. This year’s payload challenge is inspired by the Artemis missions, which seek to land the first woman and first person of color on the Moon.

Students will design a SAIL (STEMnaut Atmosphere Independent Lander) payload. It must deploy mid-air, safely return to the ground without using a parachute, and be reusable to launch the same day without repairs or modifications. The payload will contain a crew of four STEMnauts, non-living objects representing astronauts. Students will choose metrics to determine the endurance of the lander, considering acceptable descent and landing parameters.

University/college teams are required to meet the 2024 payload requirements set by NASA, but middle/high school teams have the option to tackle the same challenge or design their own payload experiment.

Student teams and attendees of NASA’s 2023 Student Launch competition observe a rocket take flight near NASA’s Marshall Space Flight Center in Huntsville, Alabama, April 2023.
Student teams and attendees of NASA’s 2023 Student Launch competition observe a rocket take flight near NASA’s Marshall Space Flight Center.
NASA

Student teams will undergo detailed reviews by NASA personnel to ensure the safety and feasibility of their rocket and payload designs. All teams must declare their rocket’s targeted altitude for final launch day during a preliminary design review. The team closest to their target will win the Altitude Award, just one of multiple awards presented to deserving teams at the end of the competition. Other awards include overall winner, vehicle design, experiment design, social media presence, and more.

In addition to the engineering and science side of the competition, students must also participate in outreach efforts such as engaging with local schools and maintaining effective social media accounts. Student Launch is an all-encompassing challenge and aims to prepare the next generation for the professional world of space exploration.

The competition is managed by Marshall’s Office of STEM Engagement (OSTEM). Additional funding and support are provided by NASA’s OSTEM via the Next Gen STEM project, NASA’s Space Operations Mission Directorate, Northrup Grumman, National Space Club Huntsville, American Institute of Aeronautics and Astronautics, National Association of Rocketry, Relativity Space, and Bastion Technologies.

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Racers Run, Bike, Run to Beat the Space Station in Annual Duathlon

On the morning of Sept. 30, 160 athletes ran and biked across NASA’s Marshall Space Flight Center and Redstone Arsenal in a race to beat the International Space Station. The annual “Racin’ the Station” duathlon is a run-bike-run event where participants try to complete the course faster than it takes the space station to complete one Earth orbit, which is every 91 minutes, 12 seconds.

Organizers track the starting location of the space station at the race start, and a costumed pacer keeps up with the station time on the course as a visual marker for participants to stay ahead of. Before the race, organizers drew a to-scale Space Launch System Block 1 rocket in chalk onto the Activities Building parking lot near the race transition area. The race began in 2012, and this year was the 11th running (the event did not occur in 2020 due to the pandemic).

Racers competed to beat the International Space Station in the annual “Racin’ the Station” duathlon Sept. 30 at Marshall Space Flight Center. The goal of the race is to complete the course faster than the station takes to complete one Earth orbit, or just over 90 minutes.
Racers competed to beat the International Space Station in the annual “Racin’ the Station” duathlon Sept. 30 at Marshall Space Flight Center. The goal of the race is to complete the course faster than the station takes to complete one Earth orbit, or just over 90 minutes.
Credits: NASA/Mick Speer

“Racin’ the Station” is not just an athletic event,” said race director and Marshall engineer Kent Criswell. “I try to also focus on educating the community about what Marshall is doing. For example, the water aid station on the run course – I call it the ECLSS (Environmental Control and Life Support System) station, but I also assure them that the water is not recycled urine from astronauts! It is a great event for any geek in the southeast — people drive all the way from Birmingham and Nashville to compete.”

The event began at 7:50 a.m. with an opening ceremony in Marshall’s Activities Building, where racers got pumped up watching the Metallica/NASA “Fuel” video for Artemis II. With the weather slowly warming, the field took off at 8:15 a.m., with a model rocket launch as the starting signal. The “station pacer” this year was dressed as Star-Lord, a superhero character appearing in the comic book and film series “Guardians of the Galaxy.”

Cyclists compete during the bicycle portion of “Racin’ the Station.”
Cyclists compete during the bicycle portion of “Racin’ the Station.”
Credits: NASA/Mick Speer

The course is three legs: a 3.14 km run, followed by a 23 km bicycle ride, and another 3.14 km run, with the start and finish line at Marshall’s Wellness Center. Race organizers arranged the distances to coincide with the number pi, approximately 3.14.

Participants can complete the entire race as an individual, or as a relay team. Eighteen teams and 124 individual racers competed, and 92 of those beat the station this year.

Runners compete in one of the two 3.14 km runs in “Racin’ the Station.”
Runners compete in one of the two 3.14 km runs in “Racin’ the Station.”
NASA/Mick Speer

The event is organized by the Team Rocket Triathlon Club in Huntsville and by the Marshall Association, a professional employee service organization at the Marshall Center whose members include civil service employees, retirees, and contractors.

For details on the race, including course maps and distances, visit the Racin’ the Station Duathlon website. Race results can be found here.

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Psyche Mission Highlighted on ‘This Week at NASA’

NASA is targeting no earlier than Oct. 12 for the launch of its Psyche spacecraft on a 2.2-billion-mile journey to study a metal-rich asteroid of the same name. The mission is featured in “This Week @ NASA,” a weekly video program broadcast on NASA-TV and posted online.

The Psyche asteroid lies in the outer portion of the main asteroid belt between Mars and Jupiter, and may be able to tell us more about the formation of rocky planets like Earth. This is NASA’s first mission to study an asteroid that has more metal than rock or ice.

Watch live coverage of the Oct. 12 Psyche launch beginning at 8:30 a.m. on NASA TV.

Psyche is the 14th planetary exploration mission in NASA’s Discovery program, which is managed for the agency by NASA’s Marshall Space Flight Center. Read more about Marshall’s role in the Psyche mission.

View this and previous episodes at “This Week @NASA” on NASA’s YouTube page.

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Experience Solar Eclipse on Oct. 14

On Oct. 14, 2023, and April 8, 2024, the entire United States and millions around the world will be able to view a solar eclipse.

A map shows the 48 contiguous U.S. states with two dark bands running across it. One band, labeled "2023 Annular Solar Eclipse," crosses states from Oregon to Texas. The other band, labeled "2024 Total Solar Eclipse," crosses states from Texas to Maine.
A map showing where the Moon’s shadow will cross the U.S. during the 2023 annular solar eclipse and 2024 total solar eclipse.
Credits: NASA SVS

There are three different kinds of solar eclipses: total, annular, and partial. When the Moon is far from the Earth, its size is too small to completely cover the Sun, thus an annular eclipse is observed, like what is expected on Oct. 14. When the Moon is close to the Earth, its larger size completely covers the Sun, causing a total eclipse, which will occur on April 8, 2024. A partial eclipse occurs when the Earth, Moon, and Sun are not perfectly aligned so only a part of the Sun will appear to be covered, giving it a crescent shape. During a total or annular solar eclipse, people outside the totality/annularity paths will see a partial solar eclipse.   

From left to right, this image shows a total solar eclipse, annular solar eclipse, and partial solar eclipse.
From left to right, this image shows a total solar eclipse, annular solar eclipse, and partial solar eclipse.
NASA

Mitzi Adams, NASA Marshall Space Flight Center​ Heliophysics and Planetary Science branch assistant chief, shares her observations during the five total eclipses she has experienced. “It is like nothing you’ve ever experienced before. It’s sort of like somebody puts a bowl on top of Earth right above where you’re standing. In the middle of the day, it gets darker, but you can still see light around the rim.” Adams explains. “You can essentially observe a sunrise or sunset. The temperatures cool. The wind picks up. The birds may go to roost, or the coyotes may howl.”

During an annular eclipse like the one coming up on Oct. 14, even with the sun covered up to 90%, the sky remains fairly bright. Those in the path of annularity will have a chance to observe the famed “ring of fire” effect, but it is important to manage your expectations and to remember that solar viewing glasses will be needed during the event’s entirety.

Bill Cooke, NASA’s Meteoroid Environment Office lead and eclipse enthusiast, says he is most looking forward to the 2024 total eclipse because totality, when the sun is covered 100%, will last much longer than the last total eclipse in 2017 – up to nearly four and a half minutes.

In any of the upcoming eclipse events, in our technology-fueled world, you may also experience some electronic changes as the moon moves across Earth and the ionosphere cools.

The ionosphere forms the boundary between the Earth’s lower atmosphere – where we live and breathe – and the vacuum of space. It is formed when particles are charged, or ionized, by solar radiation. A total solar eclipse effectively “turns off” the ionosphere’s primary charging mechanism, mimicking nighttime conditions, so the many communications signals passing through the ionosphere could be disrupted.

GPS signals could produce location errors. Radio waves could change, sometimes even allowing Ham Radio operators to send or receive transmissions over longer distances.

The ionosphere is also home to many NASA satellites, including the International Space Station.

Experiencing an eclipse is one way that everyone can participate in NASA Science. Depending on your access to different types of technology (phones, laptops, telescopes), there are several NASA Citizen Science projects you can participate in that relate to the Sun’s corona and the effects of the Moon’s shadow on Earth’s upper atmosphere.

  • GLOBE Observer
    • Help monitor the conditions of clouds, water (especially as a habitat for mosquitoes), plants (trees and other land cover), and see change over time.
  • Solar Jet Hunter
    • Join the hunt for solar jets – enigmatic bursts of energy from our own star – the Sun.
  • Planet Hunters Transiting Exoplanet Survey Satellite (TESS)
    • Find planets that will help us understand how these extrasolar systems form and evolve over time
  • Eclipse Soundscapes
    • Provide multi-sensory observations and recorded sound data to study how solar eclipses affect life on Earth!    
  • HamSCI
    • Advance scientific research and understanding through amateur radio activities.
  • Radio JOVE
    • Observe and analyze natural radio emissions of Jupiter, the Sun, and our galaxy using their own easy to construct radio telescopes.
  • Sungrazer Project
    • Become a “Comet Hunter”, and immediately begin looking for new comets in the spacecraft data. 

Regardless of how you plan to experience a solar eclipse, or any solar viewing for that matter, remember to always do so safely.

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NASA’s Bennu Asteroid Sample Contains Carbon, Water

Initial studies of the 4.5-billion-year-old asteroid Bennu sample collected in space and brought to Earth by NASA show evidence of high-carbon content and water, which together could indicate the building blocks of life on Earth may be found in the rock. NASA made the news Oct. 11 from its Johnson Space Center where leadership and scientists showed off the asteroid material for the first time since it landed in September.

This finding was part of a preliminary assessment of NASA’s OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification and Security – Regolith Explorer) science team.

nelson-tagsam-shot-b.jpg?w=2048
A view of the outside of the OSIRIS-REx sample collector. Sample material from asteroid Bennu can be seen on the middle right. Scientists have found evidence of both carbon and water in initial analysis of this material. The bulk of the sample is located inside.
Photo: NASA/Erika Blumenfeld & Joseph Aebersold

“The OSIRIS-REx sample is the biggest carbon-rich asteroid sample ever delivered to Earth and will help scientists investigate the origins of life on our own planet for generations to come,” said NASA Administrator Bill Nelson. “Almost everything we do at NASA seeks to answer questions about who we are and where we come from. NASA missions like OSIRIS-REx will improve our understanding of asteroids that could threaten Earth while giving us a glimpse into what lies beyond. The sample has made it back to Earth, but there is still so much science to come – science like we’ve never seen before.”  

Although more work is needed to understand the nature of the carbon compounds found, the initial discovery bodes well for future analyses of the asteroid sample. The secrets held within the rocks and dust from the asteroid will be studied for decades to come, offering insights into how our solar system was formed, how the precursor materials to life may have been seeded on Earth, and what precautions need to be taken to avoid asteroid collisions with our home planet.

The goal of the OSIRIS-REx sample collection was 60 grams of asteroid material. Curation experts at NASA Johnson, working in new clean rooms built especially for the mission, have spent 10 days so far carefully disassembling the sample return hardware to obtain a glimpse at the bulk sample within. When the science canister lid was first opened, scientists discovered bonus asteroid material covering the outside of the collector head, canister lid, and base. There was so much extra material it slowed down the careful process of collecting and containing the primary sample.

“Our labs were ready for whatever Bennu had in store for us,” said Vanessa Wyche, director, NASA Johnson. “We’ve had scientists and engineers working side-by-side for years to develop specialized gloveboxes and tools to keep the asteroid material pristine and to curate the samples so researchers now and decades from now can study this precious gift from the cosmos.”

Within the first two weeks, scientists performed “quick-look” analyses of that initial material, collecting images from a scanning electron microscope, infrared measurements, X-ray diffraction, and chemical element analysis. X-ray computed tomography was also used to produce a 3D computer model of one of the particles, highlighting its diverse interior. This early glimpse provided the evidence of abundant carbon and water in the sample.

“As we peer into the ancient secrets preserved within the dust and rocks of asteroid Bennu, we are unlocking a time capsule that offers us profound insights into the origins of our solar system,” said Dante Lauretta, OSIRIS-REx principal investigator, University of Arizona, Tucson. “The bounty of carbon-rich material and the abundant presence of water-bearing clay minerals are just the tip of the cosmic iceberg. These discoveries, made possible through years of dedicated collaboration and cutting-edge science, propel us on a journey to understand not only our celestial neighborhood but also the potential for life’s beginnings. With each revelation from Bennu, we draw closer to unraveling the mysteries of our cosmic heritage.”

For the next two years, the mission’s science team will continue characterizing the samples and conduct the analysis needed to meet the mission’s science goals. NASA will preserve at least 70% of the sample at Johnson for further research by scientists worldwide, including future generations of scientists. As part of OSIRIS-REx’s science program, a cohort of more than 200 scientists around the world will explore the regolith’s properties, including researchers from many U.S. institutions, NASA partners JAXA (Japan Aerospace Exploration Agency), CSA (Canadian Space Agency), and other scientists from around the world. Additional samples will also be loaned later this fall to the Smithsonian Institution, Space Center Houston, and the University of Arizona for public display.

NASA’s Goddard Space Flight Center provides overall mission management, systems engineering, and the safety and mission assurance for OSIRIS-REx. Lauretta, the principal investigator, leads the science team and the mission’s science observation planning and data processing. Lockheed Martin Space in Littleton, Colorado, built the spacecraft, provided flight operations, and was responsible for capsule recovery. Goddard and KinetX Aerospace were responsible for navigating the OSIRIS-REx spacecraft. Curation for OSIRIS-REx, including processing the sample when it arrived on Earth, is taking place at NASA Johnson.

OSIRIS-REx is the third mission in NASA’s New Frontiers Program, managed by NASA’s Marshall Space Flight Center for the Science Mission Directorate at NASA Headquarters. Read more about Marshall’s role in OSIRIS-REx.

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Webb Captures an Ethereal View of NGC 346

One of the greatest strengths of NASA’s James Webb Space Telescope is its ability to give astronomers detailed views of areas where new stars are being born. The latest example, showcased in a new image from Webb’s MIRI (Mid-Infrared Instrument), is NGC 346 – the brightest and largest star-forming region in the SMC (Small Magellanic Cloud).

The SMC is a satellite galaxy of the Milky Way, visible to the unaided eye in the southern constellation Tucana. This small companion galaxy is more primeval than the Milky Way in that it possesses fewer heavy elements, which are forged in stars through nuclear fusion and supernova explosions, compared to our own galaxy.

The lower half of this image contains arcs of bluish material that form a boat-like shape. One end of these arcs points to the top right of the image, while the other end points toward the bottom left. Another plume of blue filaments expands from the center to the top left, resembling the mast of a sailboat. Within and extending beyond the boat shape are translucent curtains of pink, which appear atop the boat shape as well and cover most of the image. Stars are noticeably scarce. A couple dozen bright pink patches with six short diffraction spikes are scattered within the blue filaments. Many faint blue dots, or stars, also speckle the background, which is black or dark gray.
This new infrared image of NGC 346 from NASA’s James Webb Space Telescope’s Mid-Infrared Instrument (MIRI) traces emission from cool gas and dust. In this image blue represents silicates and sooty chemical molecules known as polycyclic aromatic hydrocarbons, or PAHs.
NASA, ESA, CSA, STScI, N. Habel (JPL). Image Processing: P. Kavanagh (Maynooth University).

Since cosmic dust is formed from heavy elements like silicon and oxygen, scientists expected the SMC to lack significant amounts of dust. However the new MIRI image, as well as a previous image of NGC 346 from Webb’s Near-Infrared Camera released in January, show ample dust within this region.

In this representative-color image, blue tendrils trace emission from material that includes dusty silicates and sooty chemical molecules known as polycyclic aromatic hydrocarbons, or PAHs. More diffuse red emission shines from warm dust heated by the brightest and most massive stars in the heart of the region. An arc at the center left may be a reflection of light from the star near the arc’s center. (Similar, fainter arcs appear associated with stars at lower left and upper right.) Lastly, bright patches and filaments mark areas with abundant numbers of protostars. The research team looked for the reddest stars, and found 1,001 pinpoint sources of light, most of them young stars still embedded in their dusty cocoons.

By combining Webb data in both the near-infrared and mid-infrared, astronomers are able to take a fuller census of the stars and protostars within this dynamic region. The results have implications for our understanding of galaxies that existed billions of years ago, during an era in the universe known as “cosmic noon,” when star formation was at its peak and heavy element concentrations were lower, as seen in the SMC.

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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      Glover, who will be the first African American on a lunar mission, thanked Marshall team members for their work with SLS and the space station. He spent 168 days in space as a flight engineer aboard the space station for Expedition 64.
      SLS Program Manager John Honeycutt, left, and acting Center Director Joseph Pelfrey, right, join the Artemis II crew for a photo at the employee event in Activities Building 4316. NASA/Charles Beason “Thank you for your work supporting our friends who are working on the space station now and for that amazing legacy that we’ve all had the opportunity to be a part of in one facet or another,” Glover said. “We’re here to do the work and be a part of this team. We hope that what we’re doing makes you proud.”
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      Artemis II Crew Signs NASA Moon Rocket Hardware at Marshall
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      In addition to signing the Orion stage adapter, Wiseman and Koch also visited the Systems Integration Lab at Marshall prior to an employee event.
      Dan Mitchell, lead SLS integrated avionics and software engineer, talks with Wiseman and Koch as they visit the Systems Integration Lab at Marshall. NASA/Charles Beason NASA is working to land the first woman and first person of color on the Moon under Artemis. SLS is part of NASA’s backbone for deep space exploration, along with the Orion spacecraft, advanced spacesuits and rovers, the Gateway in orbit around the Moon, and commercial human landing systems. SLS is the only rocket that can send Orion, astronauts, and supplies to the Moon in a single mission. Through Artemis, NASA will explore more of the lunar surface than ever before and prepare for the next giant leap: sending astronauts to Mars.
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      Monthly Brown Bag Seminars Shine Spotlight on Marshall’s Business Units
      By Jessica Barnett
      With thousands of employees across hundreds of departments and teams, there’s no shortage of cool things happening at NASA’s Marshall Space Flight Center. To help keep Marshall team members up to date, the center recently started a series of monthly brown bag seminars aimed at highlighting its business units.
      Each month features a different business unit. On Nov. 7, nearly 300 Marshall team members attended the first seminar, which focused on Marshall’s Moon/Mars Surface Technologies and Systems. In doing so, the participants learned more about the center’s strategy.
      Geologist Jennifer Edmunson, from right, discusses lunar regolith and infrastructure plans during a brown bag seminar Nov. 7 at NASA’s Marshall Space Flight Center that highlighted the center’s Moon/Mars Surface Technologies and Systems business unit. NASA/Charles Beason “We’re in between the hopes and dreams of what you might find out there or what the vision of the future on the lunar surface might look like, and what is actually practical,” said Michael Zanetti, a lunar and planetary geologist at Marshall who was also one of the speakers during the Nov. 7 seminar.
      Zanetti discussed GPS-denied LiDAR navigation systems, including KNaCK (Kinematic Navigation and Cartography Knapsack), a proof-of-concept 3D terrain mapping, navigation, and algorithm development tool that can be used to determine the layout of portions of the lunar or Martian surface even when there is no light source or GPS to guide it.
      He also talked about Marshall’s Lunar Regolith Terrain Facility – a 125-by-125-foot area covered in 500 tons of lunar regolith simulant that can be quickly modified as needed for robotics testing.
      “If we’re going to send anything to the lunar surface, we need to make sure that technology is going to be able to function when it gets there,” said Jennifer Edmunson, project manager for Marshall’s Moon-to-Mars Planetary Autonomous Construction Technology Project, or MMPACT. “Testing with regolith is important to do that, but since we don’t have enough regolith material from the Apollo missions, we rely on simulants.”
      Materials test engineer Annette Gray, far left at table, explains how participants in Marshall’s MERCRII (Metallic Environmentally Resistant Coatings Rapid Innovation Initiative) worked with other centers and NASA partners to develop a radiation-resistant coating to improve the wear resistance of mechanism joints on the lunar or Martian surface. MMPACT is currently working to determine how best to build infrastructure on the lunar surface using the regolith and resources already available there. Edmunson shared how the project aims to build landing pads and even habitats on the Moon, but that it’s important to find ways of building that can withstand the extreme temperature variations, lengthy moonquakes, and other challenges that would be faced on the lunar surface.
      Joining Edmunson and Zanetti at the seminar was Annette Gray, a materials test engineer who was part of MERCRII (Metallic Environmentally Resistant Coatings Rapid Innovation Initiative). Gray explained how the early career initiative project worked with other centers and NASA partners to develop a radiation-resistant coating to improve the wear resistance of mechanism joints on the lunar or Martian surface.
      Part of the initiative included acquiring a Planetary, Lunar, and Asteroid Natural Environment Testbed, or PLANET. Gray said the PLANET was a 2-meter-by-3-meter chamber with up to 1 ton of regolith simulant inside that could test high vacuum, low-density plasma, and various atmospheric conditions.
      Attendees at Marshall’s first brown bag seminar check out lunar regolith samples, view informational displays, and further discuss the featured topics following the seminar.NASA/Ray Osorio The seminar ended with a question-and-answer session and a chance for in-person attendees to check out regolith simulant samples.
      “It was an excellent way to showcase how the varied work we do at Marshall is enabling future NASA missions and addressing critical gaps,” said MMSTS Strategy Lead Shawn Maynor. “The excitement was palpable, and the discussion was lively. I truly feel that Marshall is in a unique position to capitalize on the evolving space industry.”
      The next brown bag seminar is set for January 2024, after the winter holiday season.
      Barnett, a Media Fusion employee, supports the Marshall Office of Communications.
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      NASA Releases Its First International Space Station Tour in Spanish
      Lee esta nota de prensa en español aquí.
      Record-breaking NASA astronaut Frank Rubio provides the agency’s first Spanish-language video tour of humanity’s home in space – the International Space Station.
      Rubio welcomes the public aboard the microgravity science laboratory in a behind-the-scenes look at living and working in space recorded during his 371-day mission aboard the space station, the longest single spaceflight in history by an American.
      The station tour is available to watch on the agency’s NASA+ streaming platform, NASA app, NASA Television, YouTube, and the agency’s website.
      Continuously inhabited for more than 23 years, the space station is a scientific platform where crew members conduct experiments across multiple disciplines of research, including Earth and space science, biology, human physiology, physical sciences, and technology demonstrations that could not be performed on Earth.
      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.
      The crew living aboard the station are the hands of thousands of researchers on the ground conducting more than 3,300 experiments in microgravity. During his record-breaking mission, Rubio spent many hours contributing to scientific activities aboard the orbiting laboratory, conducting everything from human health studies to plant research.
      Rubio returned to Earth in September, having completed approximately 5,936 orbits of the Earth and a journey of more than 157 million miles during his first spaceflight, roughly the equivalent of 328 trips to the Moon and back.
      Get the latest NASA space station news, images and features on Instagram, Facebook, and X.
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      NASA’s Dragonfly to Proceed with Final Mission Design Work
      NASA’s Dragonfly mission has been authorized to proceed with work on final mission design and fabrication – known as Phase C – during FY (fiscal year) 2024. The agency is postponing formal confirmation of the mission (including its total cost and schedule) until mid-2024, following the release of the FY 2025 President’s Budget Request.
      Earlier this year, Dragonfly – a mission to send a rotorcraft to explore Saturn’s moon Titan – passed all the success criteria of its Preliminary Design Review. The Dragonfly team conducted a re-plan of the mission based on expected funding available in FY 2024 and estimate a revised launch readiness date of July 2028. The agency will officially assess the mission’s launch readiness date in mid-2024 at the agency Program Management Council.
      Artist’s impression of Dragonfly heading off toward its next landing spot on Titan.NASA/Johns Hopkins APL/Steve Gribben “The Dragonfly team has successfully overcome a number of technical and programmatic challenges in this daring endeavor to gather new science on Titan,” said Nicola Fox, associate administrator of NASA’s Science Mission Directorate at NASA Headquarters. “I am proud of this team and their ability to keep all aspects of the mission moving toward confirmation.”
      Dragonfly takes a novel approach to planetary exploration, for the first time employing a rotorcraft-lander to travel between and sample diverse sites on Titan. Dragonfly’s goal is to characterize the habitability of the moon’s environment, investigate the progression of prebiotic chemistry in an environment where carbon-rich material and liquid water may have mixed for an extended period, and even search for chemical indications of whether water-based or hydrocarbon-based life once existed on Titan.
      Dragonfly is being designed and built under the direction of the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, which manages the mission for NASA. The team includes key partners at NASA’s Goddard Space Flight Center; Lockheed Martin Space in Littleton, Colorado; Sikorsky, a Lockheed Martin company; NASA’s Ames Research Center; NASA’s Langley Research Center; Penn State University in State College, Pennsylvania; Malin Space Science Systems in San Diego, California; Honeybee Robotics in Pasadena, California; NASA’s Jet Propulsion Laboratory; CNES (Centre National d’Etudes Spatiales), the French space agency, in Paris, France; DLR (German Aerospace Center) in Cologne, Germany; and JAXA (Japan Aerospace Exploration Agency) in Tokyo, Japan.
      Dragonfly is the fourth mission in NASA’s New Frontiers Program, managed by NASA’s Marshall Space Flight Center for the Science Mission Directorate.
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      Webb Telescope: A Prominent Protostar in Perseus
      A new Picture of the Month from the NASA/ESA/CSA James Webb Space Telescope reveals intricate details of the Herbig Haro object 797, known as HH 797.
      Herbig-Haro objects are luminous regions surrounding newborn stars (known as protostars), and are formed when stellar winds or jets of gas spewing from these newborn stars form shockwaves colliding with nearby gas and dust at high speeds. HH 797, which dominates the lower half of the image, is located close to the young open star cluster IC 348, which is located near the eastern edge of the Perseus dark cloud complex. The bright infrared objects in the upper portion of the image are thought to host two further protostars.
      The NASA/ESA/CSA James Webb Space Telescope reveals intricate details of the Herbig Haro object 797, or HH 797. HH 797, which dominates the lower half of this image, is located close to the young open star cluster IC 348, which is located near the eastern edge of the Perseus dark cloud complex. The bright infrared objects in the upper portion of the image are thought to host two further protostars. This image was captured with Webb’s Near-InfraRed Camera (NIRCam).ESA/Webb, NASA & CSA, T. Ray (Dublin Institute for Advanced Studies) The image was captured with Webb’s NIRCam (Near-InfraRed Camera). Infrared imaging is powerful in studying newborn stars and their outflows, because the youngest stars are invariably still embedded within the gas and dust from which they are formed. The infrared emission of the star’s outflows penetrates the obscuring gas and dust, making Herbig-Haro objects ideal for observation with Webb’s sensitive infrared instruments. Molecules excited by the turbulent conditions, including molecular hydrogen and carbon monoxide, emit infrared light that Webb can collect to visualize the structure of the outflows. NIRCam is particularly good at observing the hot (thousands of degree Celsius) molecules that are excited as a result of shocks.
      Using ground-based observations, researchers have previously found that for cold molecular gas associated with HH 797, most of the red-shifted gas (moving away from us) is found to the south (bottom right), while the blue-shifted gas (moving towards us) is to the north (bottom left). A gradient was also found across the outflow, such that at a given distance from the young central star, the velocity of the gas near the eastern edge of the jet is more red-shifted than that of the gas on the western edge. Astronomers in the past thought this was due to the outflow’s rotation. In this higher resolution Webb image, however, we can see that what was thought to be one outflow is in fact made up of two almost parallel outflows with their own separate series of shocks (which explains the velocity asymmetries). The source, located in the small dark region (bottom right of center), and already known from previous observations, is therefore not a single but a double star. Each star is producing its own dramatic outflow. Other outflows are also seen in this image, including one from the protostar in the top right of center along with its illuminated cavity walls.
      HH 797 resides directly north of HH 211 (separated by approximately 30 arcseconds), which was the feature of a Webb image release in September 2023.
      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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      View the full article
    • By NASA
      NASA/Charles Beason Artemis II NASA astronauts Victor Glover, Reid Wiseman, and Christina Koch of NASA, and CSA (Canadian Space Agency) astronaut Jeremy Hansen signed the Orion stage adapter for the SLS (Space Launch System) rocket at NASA’s Marshall Space Flight Center in Huntsville, Alabama, Nov. 27. The hardware is the topmost portion of the SLS rocket that they will launch atop during Artemis II when the four astronauts inside NASA’s Orion spacecraft will venture around the Moon.

      From left, Artemis II astronauts Jeremy Hansen, Christina Koch, Victor Glover, and Reid Wiseman sign the SLS Orion stage adapter for the Artemis II mission during their visit to NASA’s Marshall Space Flight Center in Huntsville, Alabama, Nov. 27.
      Image credits: NASA/Charles Beason
      The Orion stage adapter is a small ring structure that connects NASA’s Orion spacecraft to the SLS rocket’s interim cryogenic propulsion stage and fully manufactured at Marshall. At five feet tall and weighing 1,800 pounds, the adapter is the smallest major element of the SLS rocket. During Artemis II, the adapter’s diaphragm will serve as a barrier to prevent gases created during launch from entering the spacecraft.
      NASA is working to land the first woman and first person of color on the Moon under Artemis. SLS is part of NASA’s backbone for deep space exploration, along with the Orion spacecraft, advanced spacesuits and rovers, the Gateway in orbit around the Moon, and commercial human landing systems. SLS is the only rocket that can send Orion, astronauts, and supplies to the Moon in a single mission. Through Artemis, NASA will explore more of the lunar surface than ever before and prepare for the next giant leap: sending astronauts to Mars.
      For more on NASA SLS visit:
      https://www.nasa.gov/sls
      News Media Contact
      Corinne Beckinger
      Marshall Space Flight Center, Huntsville, Ala.
      256.544.0034
      corinne.m.beckinger@nasa.gov
      View the full article
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