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The Marshall Star for November 22, 2023


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The Marshall Star for November 22, 2023

Artemis II NASA astronauts Reid Wiseman and Christina Koch of NASA, and CSA (Canadian Space Agency) astronaut Jeremy Hansen view the core stage for the SLS (Space Launch System) rocket at the agency’s Michoud Assembly Facility in New Orleans on Nov. 16.

Artemis II Astronauts View SLS Core Stage at Michoud

Artemis II NASA astronauts Reid Wiseman and Christina Koch of NASA, and CSA (Canadian Space Agency) astronaut Jeremy Hansen viewed the core stage for the SLS (Space Launch System) rocket at the agency’s Michoud Assembly Facility on Nov. 16. The three astronauts, along with NASA’s Victor Glover, will launch atop the rocket stage to venture around the Moon on Artemis II, the first crewed flight for Artemis.

Artemis II NASA astronauts Reid Wiseman and Christina Koch of NASA, and CSA (Canadian Space Agency) astronaut Jeremy Hansen view the core stage for the SLS (Space Launch System) rocket at the agency’s Michoud Assembly Facility in New Orleans on Nov. 16.
From left, Artemis II NASA astronaut Reid Wiseman, CSA (Canadian Space Agency) astronaut Jeremy Hansen, NASA astronaut Christina Koch, and Boeing’s Amanda Gertjejansen view the core stage for the SLS (Space Launch System) rocket at the agency’s Michoud Assembly Facility on Nov. 16.
NASA / Michael DeMocker

The SLS core stage, towering at 212 feet, is the backbone of the Moon rocket and includes two massive propellant tanks that collectively hold 733,000 gallons of propellant to help power the stage’s four RS-25 engines. NASA, Boeing, the core stage lead contractor, along with Aerojet Rocketdyne, an L3Harris Technologies company and the RS-25 engines lead contractor, are in the midst of conducting final integrated testing on the fully assembled rocket stage. At launch and during ascent to space, the Artemis astronauts inside NASA’s Orion spacecraft will feel the power of the rocket’s four RS-25 engines producing more than 2 million pounds of thrust for a full eight minutes. The mega rocket’s twin solid rocket boosters, which flank either side of the core stage, will each add an additional 3.6 million pounds of thrust for two minutes.

Artemis II NASA astronauts Reid Wiseman and Christina Koch of NASA, and CSA (Canadian Space Agency) astronaut Jeremy Hansen view the core stage for the SLS (Space Launch System) rocket at the agency’s Michoud Assembly Facility in New Orleans on Nov. 16.
Artemis II NASA astronauts Reid Wiseman and Christina Koch of NASA, and CSA (Canadian Space Agency) astronaut Jeremy Hansen view the core stage for the SLS (Space Launch System) rocket at the agency’s Michoud Assembly Facility in New Orleans on Nov. 16.
NASA / Michael DeMocker

The astronauts’ visit to Michoud coincided with the first anniversary of the launch of Artemis I. The uncrewed flight test of SLS and Orion was the first in a series of increasingly complex missions for Artemis as the agency works to return humans to the lunar surface and develop a long-term presence there for discovery and exploration.

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.

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Mission Success is in Our Hands: Jeramie Broadway

Mission Success is in Our Hands is a safety initiative collaboration between NASA’s Marshall Space Flight Center and Jacobs. As part of the initiative, eight Marshall team members are featured in new testimonial banners placed around the center. This is the first in a Marshall Star series profiling team members featured in the testimonial banners.

Jeramie Broadway is the center strategy lead for the Office of the Center Director.

Jeramie Broadway is center strategy lead at NASA’s Marshall Space Flight Center.
Jeramie Broadway is center strategy lead at NASA’s Marshall Space Flight Center.
NASA/Charles Beason

Before assuming this role, Broadway was senior technical assistant to the Marshall associate director, technical, from September 2021 to October 2022. In that capacity, he supported the development, coordination, and implementation of Marshall strategic planning and partnering within NASA and across industry and academia. Prior to that detail, he was the assistant manager of Marshall’s Partnerships and Formulation Office, providing strategic planning and business development support and creating new partnering and new mission opportunities for the center.

Broadway, a Dallas, Texas, native who joined NASA full-time in 2008, began his career in Marshall’s Materials and Processes Laboratory, supporting and leading production operations for the Ares I and Space Launch System program. Over the years, he served as project engineer or deputy project manager for a variety of work, including the Nuclear Cryogenic Propulsion Stage Project, for which he led development of advanced, high-temperature nuclear fuel materials. He was assistant chief engineer for launch vehicles for NASA’s Commercial Crew Program and assistant chief engineer for NASA’s Technology Demonstration Mission Program, managed for the agency at Marshall.

Question: What are some of your key responsibilities?

Broadway: Leading and implementing the center director’s strategic vision, leveraging, and integrating the strategic business units across the Marshall Center, one of NASA’s largest field installations, with nearly 7,000 on-site and near-site civil service and contractor employees and an annual budget of approximately $4 billion. Working closely in coordination and collaboration with every center organization to ensure Marshall’s planning, workflow, and business tactics align with the agency’s strategic priorities.

Question: How does your work support the safety and success of NASA and Marshall missions?

Broadway: My work as the center strategy lead is focused on the success and viability for the Marshall of the future. I work to pursue and capture programs, projects, and opportunities for Marshall to maintain ourselves as an engineering center of excellence. We work hard capturing opportunities to develop the skills, capabilities, and expertise to safely deliver on the vision and mission of the agency.

Question: What does the Mission Success Is In Our Hands initiative mean to you?

Broadway: Mission success is the responsibility of every single person at Marshall Space Flight Center, regardless of grade, position, or civil servant or support contractor. Everyone has a vital role in the success of Marshall and our ability to deliver on our mission. We all have the ability to lean forward, break down barriers, and strive for a culture that that says ‘yes, and…’.

Question: How can we work together better to achieve mission success?

Broadway: In this pursuits culture, it will take all of us to achieve the goals and objectives set forward by the agency and center leadership. We have a vibrant future with many opportunities coming our way and it will take all of us to make that vision a reality. It will take both our mission execution and our mission support organizations to get us there.

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Marshall Makes Impact at University of Alabama’s 8th Annual Space Days

By Celine Smith

Team members from NASA’s Marshall Space Flight Center participated in the 8th annual Space Days at UA (University of Alabama) on Nov 14-16, where more than 500 students met with experts from NASA and aerospace companies to learn more about the space industry.

During the three-day program, Marshall team members conducted outreach presentations and updates about the Artemis missions, HLS (Human Landing System), and other NASA programs, as well as how students can get involved in NASA’s internship program.

NASA astronaut Bob Hines delivers a presentation entitled, “An Astronaut’s Journey,” during the 8th annual Space Days at the UA on Nov. 16.
NASA astronaut Bob Hines delivers a presentation entitled, “An Astronaut’s Journey,” during the 8th annual Space Days at the UA on Nov. 16.
Matthew Wood

Kicking off the event was Aaron Houin, an engineer on the aerospace vehicle design and mission analysis team at Marshall. Houin delivered a detailed presentation on orbital mechanics and vehicle properties. Houin is no stranger to the classroom, as he is currently earning his doctorate at UA’s Astrodynamics and Space Research Laboratory and was eager to give back to his alma mater.

“Having been in their position studying the same theories, I emphasized how their coursework directly applies to physics-based modeling and trajectory design,” Houin said. “I’m hopeful sharing my experiences of transitioning from the classroom to the workplace will help others find similar success.”

The Marshall team also conducted an hour-long panel discussion and Q&A segment allowing students to learn more about the fields of aerospace and aeronautic research. Panelists included Christy Gattis, cross-program integration lead, and Kent Criswell, lead systems engineer, both representing the HLS team, as well as Tim Smith, senior mission manager of the TDM (Technology Demonstration Missions) program.

From left, Tim Smith, senior mission manager of the Technology Demonstration Missions Program, joins Human Landing System team members Christy Gattis, cross-program integration lead, and Kent Criswell, lead systems engineer, in speaking with attendees following a NASA panel discussion at the University of Alabama Space Days on Nov. 16.
From left, Tim Smith, senior mission manager of the Technology Demonstration Missions Program, joins Human Landing System team members Christy Gattis, cross-program integration lead, and Kent Criswell, lead systems engineer, in speaking with attendees following a NASA panel discussion at the University of Alabama Space Days on Nov. 16.
NASA/Christopher Blair

During the panel discussion, attendees were treated with a surprise guest speaker as Eric Vanderslice, stages structures sub element lead with SLS (Space Launch System), connected virtually from the Michoud Assembly Facility. Vanderslice shared insight about “America’s Rocket Factory” and progress for the agency’s Artemis II missions, including the recent installation of all four RS-25 engines onto the 212-ft-tall SLS core stage.

UA students also received a Tech Talk presentation focused on the SCaN (Space Communications and Navigation) program and related internship opportunities from team members from NASA’s Glenn Research Center and NASA Headquarters. Panelists included Dawn Brooks, program specialist at NASA Headquarters; Timothy Gallagher, senior project lead, and Molly Kearns, digital media specialist, all three representing SCaN’s Policy and Strategic Communications office.

And in true “One NASA” collaboration, joining the Glenn contingency for this Tech Talk was once again, Tim Smith, providing related updates on the Deep Space Optical Communications and the Laser Communications Relay Demonstration experiments.

Holly Ellis, communication specialist, and Tim Smith, senior mission manager, both of the Technology Demonstration Missions Program, speak with students during Space Days at the University of Alabama on Nov. 15.
Holly Ellis, communication specialist, and Tim Smith, senior mission manager, both of the Technology Demonstration Missions Program, speak with students during Space Days at the University of Alabama on Nov. 15.
NASA/Christopher Blair

The annual Space Days event concluded with NASA astronaut Bob Hines delivering a special presentation entitled, “An Astronaut’s Journey” to nearly 100 students, staff and industry partners. Hines completed his first spaceflight as a mission specialist for NASA’s SpaceX Crew-4 mission, serving as flight engineer of Expedition 67/68 aboard the International Space Station. 

Space Days is hosted by the UA College of Engineering and their staff shared how crucial it is to have support from aerospace industry partners willing to visit campus and meet students. Key partners exhibiting and presenting included Lockheed Martin, United Launch Alliance, Alabama Space Grant Consortium, and others.

“By the time our students attend a career fair, apply for an internship, or pursue cooperative education, they will have learned about these companies in a smaller setting and begin to consider the many pathways to success,” said Tru Livaudais, director of external affairs for UA College of Engineering. “This event offers all UA students – regardless of majors and specialties – a chance to explore future career possibilities and how to be a part of the cutting-edge research and opportunities in the space industry.”

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

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NASA Telescope Data Becomes Music You Can Play

For millennia, musicians have looked to the heavens for inspiration. Now a new collaboration is enabling actual data from NASA telescopes to be used as the basis for original music that can be played by humans.

Since 2020, the “sonification” project at NASA’s Chandra X-ray Center has translated the digital data taken by telescopes into notes and sounds. This process allows the listener to experience the data through the sense of hearing instead of seeing it as images, a more common way to present astronomical data.

The Galactic Center sonification, using data from NASA’s Chandra, Hubble and Spitzer space telescopes, has been translated into a new composition with sheet music and score. Working with a composer, this soundscape can be played by musicians.
The Galactic Center sonification, using data from NASA’s Chandra, Hubble, and Spitzer space telescopes, has been translated into a new composition with sheet music and score. Working with a composer, this soundscape can be played by musicians. The full score and sheet music for individual instruments is available at: https://chandra.si.edu/sound/symphony.html
Composition: NASA/CXC/SAO/Sophie Kastner

A new phase of the sonification project takes the data into different territory. Working with composer Sophie Kastner, the team has developed versions of the data that can be played by musicians.

“It’s like a writing a fictional story that is largely based on real facts,” said Kastner. “We are taking the data from space that has been translated into sound and putting a new and human twist on it.”

This pilot program focuses on data from a small region at the center of our Milky Way galaxy where a supermassive black hole resides. NASA’s Chandra X-ray Observatory, Hubble Space Telescope, and retired Spitzer Space Telescope have all studied this area, which spans about 400 light-years across.

“We’ve been working with these data, taken in X-ray, visible, and infrared light, for years,” said Kimberly Arcand, Chandra visualization and emerging technology scientist. “Translating these data into sound was a big step, and now with Sophie we are again trying something completely new for us.”

In the data sonification process, computers use algorithms to mathematically map the digital data from these telescopes to sounds that humans can perceive. Human musicians, however, have different capabilities than computers.

Kastner chose to focus on small sections of the image in order to make the data more playable for people. This also allowed her to create spotlights on certain parts of the image that are easily overlooked when the full sonification is played.

“I like to think of it as creating short vignettes of the data, and approaching it almost as if I was writing a film score for the image,” said Kastner. “I wanted to draw listener’s attention to smaller events in the greater data set.”

A musical ensemble performs soundscape that composer Sophie Katsner created using data sonifications from NASA’s Chandra, Hubble and Spitzer space telescopes. Based in Montreal, Ensemble Éclat is dedicated to the performance of contemporary classical music and promoting the works of emerging composers. (NASA/CXC/A. Jubett & Priam David)

The result of this trial project is a new composition based upon and influenced by real data from NASA telescopes, but with a human take.

“In some ways, this is just another way for humans to interact with the night sky just as they have throughout recorded history,” says Arcand. “We are using different tools but the concept of being inspired by the heavens to make art remains the same.”

Kastner hopes to expand this pilot composition project to other objects in Chandra’s data sonification collection. She is also looking to bring in other musical collaborators who are interested in using the data in their pieces.

Sophie Kastner’s Galactic Center piece is entitled “Where Parallel Lines Converge.” If you are a musician who wants to try playing this sonification at home, check out the sheet music at: https://chandra.si.edu/sound/symphony.html.

The piece was recorded by Montreal based Ensemble Éclat conducted by Charles-Eric LaFontaine on July 19, 2023, at McGill University.

NASA’s Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory’s Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.

Read more from NASA’s Chandra X-ray Observatory.

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Dietitian Rachel Brown Speaker for Nov. 28 Marshall Association Event

Rachel Brown, registered dietitian and certified diabetes care and education specialist, will be the guest speaker for the Marshall Association Speaker Series on Nov. 28.

The event will be 12-1 p.m. The event is free to attend and open to everyone via Teams. NASA Marshall Space Flight Center team members can attend in Building 4221, Conference Room 1103. The meeting topic follows this year’s theme of Breaking Boundaries.

Rachel Brown, registered dietitian and certified diabetes care and education specialist, will be the guest speaker for the Marshall Association Speaker Series on Nov. 28.
Rachel Brown, registered dietitian and certified diabetes care and education specialist, will be the guest speaker for the Marshall Association Speaker Series on Nov. 28.
NASA

A mom of two and a Huntsville resident since 2016, Brown is the owner of Rocket City Dietitian social media channels, where she focuses on promoting local food, fun, and fitness available in the Rocket City. She has a monthly TV segment on TN Valley Living promoting the local food scene and is a regular contributor to Huntsville Magazine, We Are Huntsville, and VisitHuntsville.org.

Email the Marshall Association for questions about the event. For more information on the Marshall Association and how to join, team members can visit their page on Inside Marshall.

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Cube Quest Concludes: Wins, Lessons Learned from Centennial Challenge

By Savannah Bullard

Artemis I launched from NASA’s Kennedy Space Center on Nov. 16, 2022, penning a new era of space exploration and inching the agency closer to sending the first woman and first person of color to the lunar surface.

Aboard the Space Launch System (SLS) rocket were 10 small satellites, no bigger than shoeboxes, whose goal was to detach and capably perform operations near and beyond the Moon. One of those satellites was a product of the Cube Quest Challenge, a NASA-led prize competition that asked citizen innovators to design, build, and deliver flight-qualified satellites called CubeSats that could perform its mission independently of the Artemis I mission.

The Orion Stage Adapter for Artemis I sits below as a large circle that has CubeSats secured along the inside yellow part of it.
Small satellites, called CubeSats, are shown secured inside NASA’s Orion stage adapter at NASA’s Kennedy Space Center on Aug. 5, 2021. One of these CubeSats belonged to Team Miles, one of the three finalists in the Cube Quest Centennial Challenge. The ring-shaped stage adapter was connected to the Space Launch System’s Interim Cryogenic Propulsion Stage, with the Orion spacecraft secured on top. The CubeSats’ mission was to detach from the stage adapter, then fly near and beyond the Moon to conduct a variety of science experiments and technology demonstrations to expand our knowledge of the lunar surface during the Artemis I mission.
NASA/Cory Huston

Cube Quest is the agency’s first in-space public prize competition. Opened in 2015, the challenge began with four ground-based tournaments, which awarded almost $500,000 in prizes. Three finalists emerged from the ground competition with a ticket to hitch a ride aboard the SLS as a secondary payload – and win the rest of the competition’s $5 million prize purse, NASA’s largest-ever prize offering to date – in 2022.

Of the three finalists, Team Miles was the sole team to make the trip on Artemis I successfully. Shortly after a successful deployment in space, controllers detected downlink signals and processed them to confirm whether the CubeSat was operational. This remains the latest update for the Team Miles CubeSat.

“We’re still celebrating the many wins that were borne out of Cube Quest,” said Centennial Challenges Program Manager Denise Morris. “The intent of the challenge was to reward citizen inventors who successfully advance the CubeSat technologies needed for operations on the Moon and beyond, and I believe we accomplished this.”

Innovation rarely comes without error, but according to Challenge Manager Naveen Vetcha, who supports Centennial Challenges through Jacobs Space Exploration Group, even after everything goes as expected, there is no guarantee that scientists will reach their desired outcomes.

“Given the magnitude of what we can and do accomplish every day at NASA, it comes with the territory that not every test, proposal, or idea will come out with 100 percent success,” Vetcha said. “We have set ambitious goals, and challenging ourselves to change what’s possible will inevitably end with examples of not meeting our stretch goals. But, with each failure comes more opportunities and lessons to carry forward. In the end, our competitors created technologies that will enable affordable deep space CubeSats, which, to me, is a big win.”

Although Team Miles may have made it furthest in the Cube Quest Challenge, having launched its CubeSat as a secondary payload aboard Artemis I, the team continues to participate in the challenge long after launch.

“From Team Miles, Miles Space LLC was created and is still in business,” said Jan McKenna, Team Miles’ project manager and safety lead. “Miles Space is developing and selling the propulsion system designed for our craft to commercial aerospace companies, and we’ve expanded to be able to create hardware for communications along with our CubeSat developments.”

The next steps for Miles Space LLC include seeing through their active patent applications, establishing relationships with potential clients, and continuing to hunt for a connection with their flying CubeSat. Another finalist team, Cislunar Explorers, is currently focused on using their lessons learned to benefit the global small satellite community.

“I utilized the contacts I made through Cube Quest and the other Artemis Secondary Payloads for my thesis research,” said Aaron Zucherman, Cislunar Explorers’ project manager. “This has enabled me to find partnerships and consulting work with other universities and companies where I have shared my experiences learning the best ways to build interplanetary CubeSats.”

This challenge featured teams from diverse educational and commercial backgrounds. Several team members credited the challenge as a catalyst in their graduate thesis or Ph.D. research, but one young innovator says Cube Quest completely redirected his entire career trajectory.

Project Selene team lead, Braden Oh, competed with his peers at La Cañada High School in La Cañada, California. Oh’s team eventually caught the attention of Kerri Cahoy at the Massachusetts Institute of Technology, and the designs were similar enough that Cahoy invited the two teams to merge. The exposure gained through this partnership was a powerful inspiration for Oh and his peers.

“I originally intended to apply to college as a computer science major, but my experiences in Cube Quest inspired me to study engineering instead,” Oh said. “I saw similar stories unfold for a number of my teammates; one eventually graduated from MIT and another now works for NASA.”

Cube Quest is managed out of NASA’s Ames Research Center. The competition is a part of NASA’s Centennial Challenges, which is housed at the agency’s Marshall Space Flight Center. Centennial Challenges is a part of NASA’s Prizes, Challenges, and Crowdsourcing program in the Space Technology Mission Directorate.

Bullard, a Manufacturing Technical Solutions Inc. employee, supports the Marshall Office of Communications.

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The Heat is On! NASA’s ‘Flawless’ Heat Shield Demo Passes the Test

A little more than a year ago, a NASA flight test article came screaming back from space at more than 18,000 mph, reaching temperatures of nearly 2,700 degrees Fahrenheit before gently splashing down in the Pacific Ocean. At that moment, it became the largest blunt body – a type of reentry vehicle that creates a heat-deflecting shockwave – ever to reenter Earth’s atmosphere.

The Low-Earth Orbit Flight Test of an Inflatable Decelerator, or LOFTID, launched Nov. 10, 2022, aboard a ULA (United Launch Alliance) Atlas V rocket and successfully demonstrated an inflatable heat shield. Also known as a Hypersonic Inflatable Aerodynamic Decelerator, or HIAD, aeroshell, this technology could allow larger spacecraft to safely descend through the atmospheres of celestial bodies like Mars, Venus, and even Saturn’s moon, Titan.

Low-Orbit Flight Test of an Inflatable Decelerator (LOFTID) on a ship deck after reentry after the demo on November 10, 2022.
The Low-Earth Orbit Flight Test of an Inflatable Decelerator, or LOFTID, spacecraft is pictured after its atmospheric re-entry test in November 2022.
NASA/Greg Swanson

“Large-diameter aeroshells allow us to deliver critical support hardware, and potentially even crew, to the surface of planets with atmospheres,” said Trudy Kortes, director of Technology Demonstrations at NASA Headquarters. “This capability is crucial for the nation’s ambition of expanding human and robotic exploration across our solar system.”

NASA has been developing HIAD technologies for over a decade, including two smaller scale suborbital flight tests before LOFTID. In addition to this successful tech demo, NASA is investigating future applications, including partnering with commercial companies to develop technologies for small satellite reentry, aerocapture, and cislunar payloads.

“This was a keystone event for us, and the short answer is: It was highly successful,” said LOFTID Project Manager Joe Del Corso. “Our assessment of LOFTID concluded with the promise of what this technology may do to empower the exploration of deep space.”

Due to the success of the LOFTID tech demo, NASA announced under its Tipping Point program that it would partner with ULA to develop and deliver the “next size up,” a larger 12-meter HIAD aeroshell for recovering the company’s Vulcan engines from low Earth orbit for reuse.

The LOFTID team recently held a post-flight analysis assessment of the flight test at NASA’s Langley Research Center. Their verdict?

Upon recovery, the team discovered LOFTID appeared pristine, with minimal damage, meaning its performance was, as Del Corso puts it, “Just flawless.”

View some interesting visual highlights from LOFTID’s flight test.

LOFTID splashed down in the Pacific Ocean several hundred miles off the east coast of Hawaii and only about eight miles from the recovery ship’s bow – almost exactly as modeled. A crew got on a small boat and retrieved and hoisted LOFTID onto the recovery ship.

“The LOFTID mission was important because it proved the cutting-edge HIAD design functioned successfully at an appropriate scale and in a relevant environment,” said Tawnya Laughinghouse, manager of the TDM (Technology Demonstrations Missions) program office at NASA’s Marshall Space Flight Center.

Marshall supported the Langley-led LOFTID project, providing avionics flight hardware, including the data acquisition system, the inertial measurement unit, and six camera pods. Marshall engineers also performed thermal and fluids analyses and modeling in support of the LOFTID re-entry vehicle inflation system and aeroshell designs.

The LOFTID demonstration was a public private-partnership with ULA funded by STMD and managed by the Technology Demonstration Mission Program, executed by NASA Langley with contributions from across NASA centers. Multiple U.S. small businesses contributed to the hardware. NASA’s Launch Services Program was responsible for NASA’s oversight of launch operations.

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      Laura Betz – laura.e.betz@nasa.gov
      NASA’s Goddard Space Flight Center, Greenbelt, Md.
      Ann Jenkins – jenkins@stsci.edu
      Space Telescope Science Institute, Baltimore, Md.
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      Last Updated Sep 04, 2025 Related Terms
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    • By NASA
      NASA/Nichole Ayers On July 26, 2025, NASA astronaut Nichole Ayers took this long-exposure photograph – taken over 31 minutes from a window inside the International Space Station’s Kibo laboratory module – capturing the circular arcs of star trails.
      In its third decade of continuous human presence, the space station has a far-reaching impact as a microgravity lab hosting technology, demonstrations, and scientific investigations from a range of fields. The research done on the orbiting laboratory will inform long-duration missions like Artemis and future human expeditions to Mars.
      Image credit: NASA/Nichole Ayers
      View the full article
    • By NASA
      Explore Hubble Hubble Home Overview About Hubble The History of Hubble Hubble Timeline Why Have a Telescope in Space? Hubble by the Numbers At the Museum FAQs Impact & Benefits Hubble’s Impact & Benefits Science Impacts Cultural Impact Technology Benefits Impact on Human Spaceflight Astro Community Impacts Science Hubble Science Science Themes Science Highlights Science Behind Discoveries Universe Uncovered Hubble’s Partners in Science AI and Hubble Science Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Astronaut Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts Multimedia Images Videos Sonifications Podcasts e-Books Online Activities 3D Hubble Models Lithographs Fact Sheets Posters Hubble on the NASA App Glossary News Hubble News Social Media Media Resources More 35th Anniversary Online Activities 2 min read
      Hubble Homes in on Galaxy’s Star Formation
      This NASA/ESA Hubble Space Telescope image features the asymmetric spiral galaxy Messier 96. ESA/Hubble & NASA, F. Belfiore, D. Calzetti This NASA/ESA Hubble Space Telescope image features a galaxy whose asymmetric appearance may be the result of a galactic tug of war. Located 35 million light-years away in the constellation Leo, the spiral galaxy Messier 96 is the brightest of the galaxies in its group. The gravitational pull of its galactic neighbors may be responsible for Messier 96’s uneven distribution of gas and dust, asymmetric spiral arms, and off-center galactic core.
      This asymmetric appearance is on full display in the new Hubble image that incorporates data from observations made in ultraviolet, near infrared, and visible/optical light. Earlier Hubble images of Messier 96 were released in 2015 and 2018. Each successive image added new data, building up a beautiful and scientifically valuable view of the galaxy.
      The 2015 image combined two wavelengths of optical light with one near infrared wavelength. The optical light revealed the galaxy’s uneven form of dust and gas spread asymmetrically throughout its weak spiral arms and its off-center core, while the infrared light revealed the heat of stars forming in clouds shaded pink in the image.
      The 2018 image added two more optical wavelengths of light along with one wavelength of ultraviolet light that pinpointed areas where high-energy, young stars are forming.
      This latest version offers us a new perspective on Messier 96’s star formation. It includes the addition of light that reveals regions of ionized hydrogen (H-alpha) and nitrogen (NII). This data helps astronomers determine the environment within the galaxy and the conditions in which stars are forming. The ionized hydrogen traces ongoing star formation, revealing regions where hot, young stars are ionizing the gas. The ionized nitrogen helps astronomers determine the rate of star formation and the properties of gas between stars, while the combination of the two ionized gasses helps researchers determine if the galaxy is a starburst galaxy or one with an active galactic nucleus.
      The bubbles of pink gas in this image surround hot, young, massive stars, illuminating a ring of star formation in the galaxy’s outskirts. These young stars are still embedded within the clouds of gas from which they were born. Astronomers will use the new data in this image to study how stars are form within giant dusty gas clouds, how dust filters starlight, and how stars affect their environments.
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      Explore the Night Sky: Messier 96

      Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact:
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      NASA’s Goddard Space Flight Center, Greenbelt, MD
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      Last Updated Aug 29, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
      Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center Hubble Space Telescope Spiral Galaxies Stars The Universe Keep Exploring Discover More Topics From Hubble
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    • By NASA
      This graphic features data from NASA’s Chandra X-ray Observatory of the Cassiopeia A (Cas A) supernova remnant that reveals that the star’s interior violently rearranged itself mere hours before it exploded. The main panel of this graphic is Chandra data that shows the location of different elements in the remains of the explosion: silicon (represented in red), sulfur (yellow), calcium (green) and iron (purple). The blue color reveals the highest-energy X-ray emission detected by Chandra in Cas A and an expanding blast wave. The inset reveals regions with wide ranges of relative abundances of silicon and neon. This data, plus computer modeling, reveal new insight into how massive stars like Cas A end their lives.X-ray: NASA/CXC/Meiji Univ./T. Sato et al.; Image Processing: NASA/CXC/SAO/N. Wolk The inside of a star turned on itself before it spectacularly exploded, according to a new study from NASA’s Chandra X-ray Observatory. Today, this shattered star, known as the Cassiopeia A supernova remnant, is one of the best-known, well-studied objects in the sky.
      Over three hundred years ago, however, it was a giant star on the brink of self-destruction. The new Chandra study reveals that just hours before it exploded, the star’s interior violently rearranged itself. This last-minute shuffling of its stellar belly has profound implications for understanding how massive stars explode and how their remains behave afterwards.
      Cassiopeia A (Cas A for short) was one of the first objects the telescope looked at after its launch in 1999, and astronomers have repeatedly returned to observe it.
      “It seems like each time we closely look at Chandra data of Cas A, we learn something new and exciting,” said Toshiki Sato of Meiji University in Japan who led the study. “Now we’ve taken that invaluable X-ray data, combined it with powerful computer models, and found something extraordinary.”
      As massive stars age, increasingly heavy elements form in their interiors by nuclear reactions, creating onion-like layers of different elements. Their outer layer is mostly made of hydrogen, followed by layers of helium, carbon and progressively heavier elements – extending all the way down to the center of the star. 
      Once iron starts forming in the core of the star, the game changes. As soon as the iron core grows beyond a certain mass (about 1.4 times the mass of the Sun), it can no longer support its own weight and collapses. The outer part of the star falls onto the collapsing core, and rebounds as a core-collapse supernova.
      The new research with Chandra data reveals a change that happened deep within the star at the very last moments of its life. After more than a million years, Cas A underwent major changes in its final hours before exploding.
      “Our research shows that just before the star in Cas A collapsed, part of an inner layer with large amounts of silicon traveled outwards and broke into a neighboring layer with lots of neon,” said co-author Kai Matsunaga of Kyoto University in Japan. “This is a violent event where the barrier between these two layers disappears.”
      This upheaval not only caused material rich in silicon to travel outwards; it also forced material rich in neon to travel inwards. The team found clear traces of these outward silicon flows and inward neon flows in the remains of Cas A’s supernova remnant. Small regions rich in silicon but poor in neon are located near regions rich in neon and poor in silicon. 
      The survival of these regions not only provides critical evidence for the star’s upheaval, but also shows that complete mixing of the silicon and neon with other elements did not occur immediately before or after the explosion. This lack of mixing is predicted by detailed computer models of massive stars near the ends of their lives.
      There are several significant implications for this inner turmoil inside of the doomed star. First, it may directly explain the lopsided rather than symmetrical shape of the Cas A remnant in three dimensions. Second, a lopsided explosion and debris field may have given a powerful kick to the remaining core of the star, now a neutron star, explaining the high observed speed of this object.
      Finally, the strong turbulent flows created by the star’s internal changes may have promoted the development of the supernova blast wave, facilitating the star’s explosion.
      “Perhaps the most important effect of this change in the star’s structure is that it may have helped trigger the explosion itself,” said co-author Hiroyuki Uchida, also of Kyoto University. “Such final internal activity of a star may change its fate—whether it will shine as a supernova or not.”
      These results have been published in the latest issue of The Astrophysical Journal and are available online.
      To learn more about Chandra, visit:
      https://science.nasa.gov/chandra
      Read more from NASA’s Chandra X-ray Observatory Learn more about the Chandra X-ray Observatory and its mission here:
      https://www.nasa.gov/chandra
      https://chandra.si.edu
      Visual Description
      This release features a composite image of Cassiopeia A, a donut-shaped supernova remnant located about 11,000 light-years from Earth. Included in the image is an inset closeup, which highlights a region with relative abundances of silicon and neon.
      Over three hundred years ago, Cassiopeia A, or Cas A, was a star on the brink of self-destruction. In composition it resembled an onion with layers rich in different elements such as hydrogen, helium, carbon, silicon, sulfur, calcium, and neon, wrapped around an iron core. When that iron core grew beyond a certain mass, the star could no longer support its own weight. The outer layers fell into the collapsing core, then rebounded as a supernova. This explosion created the donut-like shape shown in the composite image. The shape is somewhat irregular, with the thinner quadrant of the donut to the upper left of the off-center hole.
      In the body of the donut, the remains of the star’s elements create a mottled cloud of colors, marbled with red and blue veins. Here, sulfur is represented by yellow, calcium by green, and iron by purple. The red veins are silicon, and the blue veins, which also line the outer edge of the donut-shape, are the highest energy X-rays detected by Chandra and show the explosion’s blast wave.
      The inset uses a different color code and highlights a colorful, mottled region at the thinner, upper left quadrant of Cas A. Here, rich pockets of silicon and neon are identified in the red and blue veins, respectively. New evidence from Chandra indicates that in the hours before the star’s collapse, part of a silicon-rich layer traveled outwards, and broke into a neighboring neon-rich layer. This violent breakdown of layers created strong turbulent flows and may have promoted the development of the supernova’s blast wave, facilitating the star’s explosion. Additionally, upheaval in the interior of the star may have produced a lopsided explosion, resulting in the irregular shape, with an off-center hole (and a thinner bite of donut!) at our upper left.
      News Media Contact
      Megan Watzke
      Chandra X-ray Center
      Cambridge, Mass.
      617-496-7998
      mwatzke@cfa.harvard.edu
      Corinne Beckinger
      Marshall Space Flight Center, Huntsville, Alabama
      256-544-0034
      corinne.m.beckinger@nasa.gov
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      Last Updated Aug 28, 2025 EditorLee MohonContactCorinne M. Beckingercorinne.m.beckinger@nasa.govLocationMarshall Space Flight Center Related Terms
      Chandra X-Ray Observatory General Marshall Astrophysics Marshall Space Flight Center Supernova Remnants Supernovae The Universe Explore More
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    • By USH
      NASA’s 1991 Discovery shuttle video shows UFOs making impossible maneuvers, evading a possible Star Wars railgun test. Evidence of secret tech? 

      In September 1991, NASA’s Space Shuttle Discovery transmitted live video that has since become one of the most debated UFO clips ever recorded. The footage, later analyzed by independent researchers, shows glowing objects in orbit performing maneuvers far beyond the limits of known physics. 
      One object appears over Earth’s horizon, drifts smoothly, then suddenly reacts to a flash of light by accelerating at impossible speeds, estimated at over 200,000 mph while withstanding forces of 14,000 g’s. NASA officially dismissed the anomalies as ice particles or debris, but side by side comparisons with actual orbital ice show key differences: the objects make sharp turns, sudden accelerations, and fade in brightness in ways consistent with being hundreds of miles away, not near the shuttle. 
      Image analysis expert Dr. Mark Carlotto confirmed that at least one object was located about 1,700 miles from the shuttle, placing it in Earth’s atmosphere. At that distance, the object would be too large and too fast to be dismissed as ice or space junk. 
      The flash and two streaks seen in the video resemble the Pentagon’s “Brilliant Pebbles” concept, a railgun based missile defense system tested in the early 1990s. Researchers suggest the shuttle cameras may have accidentally, or deliberately, captured a live Star Wars weapons test in orbit. 
      The UFO easily evaded the attack, leading some to conclude that it was powered by a form of hyperdimensional technology capable of altering gravity. 
      Notably, following this 1991 incident, all subsequent NASA shuttle external camera feeds were censored or delayed, raising speculation that someone inside the agency allowed the extraordinary footage to slip out.
        View the full article
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