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The Marshall Star for February 7, 2024


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The Marshall Star for February 7, 2024

Joseph Pelfrey talks during a 2023 all-hands meeting at Marshall.

NASA Administrator Announces New Marshall Space Flight Center Director

NASA Administrator Bill Nelson on Feb. 5 named Joseph Pelfrey director of the agency’s Marshall Space Flight Center, effective immediately. Pelfrey has served as acting center director since July 2023.

“Joseph is a respected leader who shares the passion for innovation and exploration at NASA Marshall. As center director, he will lead the entire Marshall workforce, which includes a world-renowned team of scientists, engineers, and technologists who have a hand in nearly every NASA mission,” said Nelson. “I am confident that under Joseph’s leadership, Marshall will continue to make critical advancements supporting Artemis and Moon to Mars that will benefit all humanity.” 

Marshall Space Flight Center Director Joseph Pelfrey.
Marshall Space Flight Center Director Joseph Pelfrey.
NASA

NASA Marshall is one of the agency’s largest field centers, and manages NASA’s Michoud Assembly Facility, where some of the largest elements of the SLS (Space Launch System) rocket and Orion spacecraft for the Artemis campaign are manufactured. The center also is responsible for the oversight and execution of an approximately $5 billion portfolio comprised of human spaceflight, science, and technology development efforts. Its workforce consists of nearly 7,000 employees, both civil servants and contractors. 

“Marshall is renowned for its expertise in exploration and scientific discovery, and I am honored and humbled to be chosen to lead the center into the future,” said Pelfrey. “We will continue to shape the future of human space exploration by leading SLS and human landing system development for Artemis and leveraging our capabilities to make critical advancements in human landing and cargo systems, habitation and transportation systems, advanced manufacturing, mission operations, and cutting-edge science and technology missions.”

Pelfrey talks during a 2023 all-hands meeting at Marshall.
Pelfrey talks during a 2023 all-hands meeting at Marshall.
NASA/Charles Beason

Prior to joining NASA, Pelfrey worked in industry, supporting development of space station payload hardware. He began his NASA career as an aerospace engineer in the Science and Mission Systems Office, going on to serve in various leadership roles within the International Space Station Program, the Marshall Engineering Directorate and the SLS Spacecraft/Payload Integration and Evolution Office. He also served as manager for the Commercial Orbital Transportation Services Project at Marshall and the Exploration and Space Transportation Development Office in the Flight Programs and Partnerships Office.

Appointed to the Senior Executive Service in 2016, Pelfrey served as the associate director for operations in Engineering, later becoming deputy manager and subsequently manager for Marshall’s Human Exploration Development and Operations Office. He was appointed as Marshall’s deputy center director in April 2022.

Pelfrey received a bachelor’s degree in Aerospace Engineering from Auburn University in 2000.

Learn more about Pelfrey.

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NASA to Demonstrate Autonomous Navigation System on Moon

By Rick Smith

When the second CLPS (Commercial Lunar Payload Services) delivery is launched to the Moon in mid-February, its NASA payloads will include an experiment that could change how human explorers, rovers, and spacecraft independently track their precise location on the Moon and in cis-lunar space.

Demonstrating autonomous navigation, the Lunar Node-1 experiment, or LN-1, is a radio beacon designed to support precise geolocation and navigation observations for landers, surface infrastructure, and astronauts, digitally confirming their positions on the Moon relative to other craft, ground stations, or rovers on the move. These radio beacons also can be used in space to help with orbital maneuvers and with guiding landers to a successful touchdown on the lunar surface.

An close up image of the Lunar Node-1 payload covered in a silver wrapping to protect it in space.
Lunar Node-1, or LN-1, an autonomous navigation payload that will change how human explorers safely traverse the Moon’s surface and live and work in lunar orbit, awaits liftoff as part of Intuitive Machines’ IM-1 mission, its first under NASA’s Commercial Lunar Payload Services initiative. LN-1 was developed, built, and tested at NASA’s Marshall Space Flight Center.
NASA/Intuitive Machines

“Imagine getting verification from a lighthouse on the shore you’re approaching, rather than waiting on word from the home port you left days earlier,” said Evan Anzalone, principal investigator of LN-1 and a navigation systems engineer at NASA’s Marshall Space Flight Center. “What we seek to deliver is a lunar network of lighthouses, offering sustainable, localized navigation assets that enable lunar craft and ground crews to quickly and accurately confirm their position instead of relying on Earth.”

The system is designed to operate as part of a broader navigation infrastructure, anchored by a series of satellites in lunar orbit as being procured under NASA’s Lunar Communications Relay and Navigation Systems project. Together, future versions of LN-1 would utilize LunaNet-defined standards to provide interoperable navigation reference signals from surface beacons as well as orbital assets.

Currently, navigation beyond Earth is heavily reliant on point-to-point services provided by NASA’s Deep Space Network, an international array of giant radio antennas which transmit positioning data to interplanetary spacecraft to keep them on course. These measurements typically are relayed back to Earth and processed on the ground to deliver information back to the traveling vehicle.

But when seconds count during orbital maneuvers, or among explorers traversing uncharted areas of the lunar surface, LN-1 offers a timely improvement, Anzalone said.

The Nova-C lunar lander sits in front of an American flag with dramatic lighting against it.
IM-1, the first NASA Commercial Launch Program Services launch for Intuitive Machines’ Nova-C lunar lander, will carry multiple payloads to the Moon, including Lunar Node-1, demonstrating autonomous navigation via radio beacon to support precise geolocation and navigation among lunar orbiters, landers, and surface personnel. NASA’s CLPS initiative oversees industry development of small robotic landers and rovers to support NASA’s Artemis campaign.
NASA/Intuitive Machines

The CubeSat-sized experiment is one of six payloads included in the NASA delivery manifest for Intuitive Machines of Houston, which will be launched via a SpaceX Falcon 9 from Cape Canaveral, Florida. Designated IM-1, the launch is the company’s first for NASA’s CLPS initiative, which oversees industry development, testing, and launch of small robotic landers and rovers supporting NASA’s Artemis campaign.

The Nova-C lander is scheduled to touch down near Malapert A, a lunar impact crater in the Moon’s South Pole region.

LN-1 relies on networked computer navigation software known as MAPS (Multi-spacecraft Autonomous Positioning System). Developed by Anzalone and researchers at Marshall, MAPS was successfully tested on the International Space Station in 2018 using NASA’s Space Communications and Navigation testbed.

Engineers at Marshall conducted all structural design, thermal and electronic systems development, and integration and environmental testing of LN-1 as part of the NASA-Provided Lunar Payloads project funded by the agency’s Science Mission Directorate. Anzalone and his team delivered the payload in 2021, having performed the payload build during the COVID pandemic. Since then, they refined the operating procedures, conducted thorough testing of the integrated flight system, and in October 2023, oversaw installation of LN-1 on Intuitive Machines’ lander.

Demonstrating autonomous navigation, the Lunar Node-1 experiment, or LN-1, is a radio beacon designed to support precise geolocation and navigation observations to orbiters, landers, and surface personnel, digitally confirming their positions on the Moon relative to other craft, ground stations, or rovers on the move. The system is designed to operate as part of a broader navigation infrastructure, anchored by a series of satellites in lunar orbit as being procured under NASA’s Lunar Communications Relay and Navigation Systems project. (NASA)

The payload will transmit information briefly each day during the journey to the Moon. Upon lunar touchdown, the LN-1 team will conduct a full systems checkout and begin continuous operations within 24 hours of landing. NASA’s Deep Space Network will receive its transmissions, capturing telemetry, Doppler tracking, and other data and relaying it back to Earth. Researchers at NASA’s Jet Propulsion Laboratory and at Morehead State University in Kentucky also will monitor LN-1’s transmissions throughout the mission, which is scheduled to last approximately 10 days.

Eventually, as the technology is proven and its infrastructure expanded, Anzalone expects LN-1 to evolve from a single lighthouse on the lunar shore into a key piece of a much broader infrastructure, helping NASA evolve its navigation system into something more akin to a bustling metropolitan subway network, wherein every train is tracked in real time as it travels its complex route.

“Spacecraft, surface vehicles, base camps and exploratory digs, even individual astronauts on the lunar surface,” Anzalone said. “LN-1 could connect them all and help them navigate more accurately, creating a reliable, more autonomous lunar network.”

Marshall’s LN-1 team is already discussing future Moon to Mars applications for LN-1 with NASA’s SCaN (Space Communications and Navigation) program – which oversees more than 100 NASA and partner missions. They’re also consulting with the European Space Agency and Japan Aerospace Exploration Agency, aiding the push to unite spacefaring nations via an interconnected, interoperable global architecture.

“Eventually, these same technologies and applications we’re proving at the Moon will be vital on Mars, making those next generations of human explorers safer and more self-sufficient as they lead us out into the solar system,” Anzalone said.

NASA’s CLPS initiative enables NASA to buy a complete commercial robotic lunar delivery service from leading aerospace contractors. The provider is responsible for launch services, owns its lander design, and leads landing operations. Learn more here.

Smith, an Aeyon/MTS employee, supports the Marshall Office of Communications.

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Marshall Wraps Up Mentoring Month with Mega Meal, Mentoring Panel

By Jessica Barnett

There was no shortage of opportunities in January to learn about the benefits of mentoring from those who have experienced them firsthand. In fact, there was so much to share, team members at NASA’s Marshall Space Flight Center kept the celebration going through the first week of February.

“It was so great to see so many from our workforce out and excited about mentorship,” said Selina Salgado, who serves as the Mentoring Program coordinator at Marshall. “At every event throughout the month and when reading through the highlights, I was encouraged by the engagement and commitment that the Marshall team showed for development.”

Marshall Space Flight Center Chief Financial Officer Rhega Gordon, center, who participates in the center’s Mentorship Program, discusses the benefits of mentoring and her advice for getting the most out of a mentoring relationship during a panel event held Feb. 6 in Activities Building 4316 as part of Marshall’s celebration of National Mentoring Month. Joining her on stage are two of her mentees, program specialist Kim Henry and Marshall Sustainability Coordinator Malene McElroy.
Marshall Space Flight Center Chief Financial Officer Rhega Gordon, center, who participates in the center’s Mentorship Program, discusses the benefits of mentoring and her advice for getting the most out of a mentoring relationship during a panel event held Feb. 6 in Activities Building 4316 as part of Marshall’s celebration of National Mentoring Month. Joining her on stage are two of her mentees, program specialist Kim Henry and Marshall Sustainability Coordinator Malene McElroy.
NASA/Danielle Burleson

This year’s events included Meals with Mentors, in which team members could have lunch and chat with mentors from a variety of backgrounds and departments, and an in-person mentoring panel Feb. 6 featuring Marshall Chief Financial Officer Rhega Gordon and two of her mentees, Marshall Sustainability Coordinator Malene McElroy and program specialist Kim Henry.

Marshall also participated in the launch for AMPED (Agencywide Mentoring Pilot for Engagement & Development), which pairs mentors and mentees together using the MentorcliQ platform. Civil servants can sign up for AMPED now through Feb. 19.

Marshall team members can also participate in MERGE, a NASA-built mentoring application that allows users to create and view profiles to identify potential mentors or mentees. MERGE is recommended for casual, informal, or short-term mentoring relationships, as well as shadowing opportunities. Civil servants and contractors can sign up at any time.

Marshall Associate Center Director, Technical, Larry Leopard engages with center team members during a Meals with Mentors event Feb. 6 in Activities Building 4316. Team members were encouraged to chat with center leaders and potential mentors at the event as part of Marshall’s celebration of National Mentoring Month.
Marshall Associate Center Director, Technical, Larry Leopard engages with center team members during a Meals with Mentors event Feb. 6 in Activities Building 4316. Team members were encouraged to chat with center leaders and potential mentors at the event as part of Marshall’s celebration of National Mentoring Month.
NASA/Danielle Burleson

In addition to in-person events and showcasing new options for finding a mentor or mentee, there were weekly tips to help team members get the most out of their mentorship journey and interviews with mentors and mentees, who shared their experiences, advice, and more.

“Our hope was that employees would reengage with mentorship, find value in their current relationships, or provide resources and guidance to help those who were new to the world of mentoring,” Salgado said.

Marshall team members can start or continue their mentorship journey by visiting the Marshall Mentorship Program page on Inside Marshall.

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

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Mission Success is in Our Hands: Ashley Marlar

By Wayne Smith

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 fourth in a Marshall Star series profiling team members featured in the testimonial banners. The next Mission Success is in Our Hands Shared Experience Forum will be Feb. 22 and will feature Robert Conway, deputy director of NASA’s Safety Center. The 11:30 a.m. event will be in Activities Building 4316 for Marshall team members.

Ashley Marlar is the Jacobs Space Exploration Group team lead of Operations Engineering Support at Marshall, responsible for managing a team of four Jacobs Transportation engineers supporting the center’s Transportation and Logistics Engineering Office. Marlar and her team develop and execute detailed plans, procedures, and engineered lift analyses to transport NASA’s SLS (Space Launch System) flight hardware and test articles, as well as hardware for various other programs and projects at Marshall.

Ashley Marlar is the Jacobs Space Exploration Group Team Lead of Operations Engineering Support at NASA’s Marshall Space Flight Center, supporting the Transportation and Logistics Engineering Office.
Ashley Marlar is the Jacobs Space Exploration Group Team Lead of Operations Engineering Support at NASA’s Marshall Space Flight Center, supporting the Transportation and Logistics Engineering Office.
NASA/Charles Beason

She has worked at Marshall for eight years, including six years with Jacobs, starting her career as a transportation and logistics engineer. A native of Hazel Green, Alabama, Marlar is a graduate of the University of Alabama in Huntsville where she earned a bachelor’s degree in aerospace engineering.

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

Marlar: The thorough coordination and detailed planning of each hardware movement is absolutely critical to the safety of the hardware and the personnel handling it, and the success of the mission. We must anticipate risks and consider contingency plans. Whether it’s offloading a welded component from the delivery truck, installing a test article into a structural test stand, or shipping the SLS core stage on the barge Pegasus from NASA’s Michoud Assembly Facility to the agency’s Kennedy Space Center, we meticulously plan every step of the operation to ensure the hardware is delivered without mishaps or delays.

Question: What does the Mission Success is in Our Hands initiative mean to you?

Marlar: To me it means every individual plays a vital role in making our missions safe and successful. We all contribute to NASA’s success by bringing our unique skills and perspectives to the table. And we are all responsible for the safety of ourselves and each other by having the courage to speak up and ask questions.

Question: Do you have a story or personal experience you can share that might help others understand the significance of mission assurance or flight safety?

Marlar: One of the things we do to help ensure mission safety is perform dry runs, like dress rehearsals, for many of our major moves. For example, we utilized the core stage Pathfinder vehicle to practice our transportation methods and iron out all the little details of our procedures without risking the actual core stage flight unit. We repeatedly practiced installing the Pathfinder onto ground support equipment, lifting and rotating it from horizontal to vertical orientation, and installing it into the B2 test stand at Stennis Space Center. Then we did everything in reverse. We did this multiple times to identify any challenges, safety issues, or workflow inefficiencies we might face when it came time to perform these tasks with the real thing, and then made many procedural changes and some hardware changes to mitigate those risks and resolve numerous issues. All of this paid off in a big way when we transported, lifted, and tested the flight core stage flawlessly.

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

Marlar: Mission success is a team effort and a shared responsibility. I think it’s vital to encourage and empower everyone to speak up and share their ideas and concerns as well as hold each other accountable. We should continue to reinforce the importance of communication and engagement, particularly as we emerge from a pandemic. 

Question: Do you have anything else you’d like to share?

Marlar: My primary goal is to make sure my team gets home safe and sound at the end of the day. As important and grand as our mission is, our biggest asset is our people. We are a collective of many pieces in a large puzzle, but every piece is equally important to the whole.

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

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NASA Taps Alabama A&M University to Host Break the Ice Lunar Challenge

By Savannah Bullard

NASA has selected Alabama A&M University’s Agribition Center in Huntsville to host the final level of the agency’s Break the Ice Lunar Challenge, using indoor and outdoor space to ground test the finalists’ solutions.

The challenge opened in 2020 to find novel solutions for excavating icy lunar regolith and delivering acquired resources in extreme environmental conditions. In alignment with NASA’s Moon to Mars objectives, the challenge aims to develop technologies that could support a sustained human presence on the Moon.

An external image of the Alabama A&M University Agribition Center from the front facade. The Center is a cream-colored stone building with a curved roof, floor-to-ceiling windows, and concrete steps that lead to a covered awning, framed by deep-red structural beams above. Shrubs and crepe myrtle trees frame the foreground and steps leading up to the building. Photo courtesy of AAMU Extension
Alabama A&M University’s Agribition Center will host the final Break the Ice Lunar Challenge featuring a large dirt-based indoor arena on 40 acres of land, offering plenty of green space to build Break the Ice’s complex testing infrastructure.
Photo Courtesy: Alabama A&M University Extension

Throughout the challenge, competitors have designed, built, and independently tested robots that could theoretically withstand the harsh environments inside permanently shadowed regions of the lunar South Pole. The six finalists who succeeded in Phase 2: Level 2 of the challenge were announced in December 2023.

“We were looking for a unique set of criteria to house the Break the Ice Lunar competition, so we partnered with Jacobs Space Exploration Group in finding a facility,” said Denise Morris, NASA Centennial Challenges program manager at NASA’s Marshall Space Flight Center. “Alabama A&M is a good fit for this challenge because of the on-site capabilities they have and being close to NASA facilities makes logistics much easier.”

Located a few miles east of the Alabama A&M University campus, the Agribition (agriculture + exhibition) Center is managed by the Alabama Cooperative Extension System with support from the university and its College of Agricultural, Life, and Natural Sciences. Its indoor arena features a large dirt space, typically equipped to support rodeos and other agricultural expos. Outside, the center sits on roughly 40 acres of land, offering plenty of green space to build the competition’s complex infrastructure.

The final Phase 2: Level 3 testing will occur June 10-12, 2024. There are two components that each team will focus on mastering: excavation and transportation.

Six identically sized concrete slabs will be set up inside the arena for the finalists’ robots to dig. The slabs, measuring 300 cubic feet, will have qualities similar to a permanently shadowed crater located at the Moon’s South Pole. A gravity-offloading crane and pulley system will lift the excavators while working, simulating the one-sixth gravity experienced on the Moon.

Each team will have one hour to dig as much material as possible or until they reach the payload capacity of their excavation robot. Up to three top-performing teams will earn an opportunity to test their solution inside one of the thermal vacuum chambers located at Marshall, which can simulate the temperature and vacuum conditions at the lunar South Pole.

Outside the Agribition Center, challenge teams will take turns on a custom-built track outfitted with slopes, boulders, pebbles, rocks, and gravel to simulate the lunar surface. This volatile surface will stretch approximately 300 meters and include several twists and turns for more intermediate handling.

Each team will get one hour on the track to deliver a payload and return to the starting point. Times, distances, and pitfalls will be recorded independently.

“These two testing methods address the excavation and transportation of large quantities of icy regolith, which are some of NASA’s current top technology gaps,” said Naveen Vetcha, NASA challenge manager at Jacobs Space Exploration Group. “This competition has enabled teams to develop lightweight, energy efficient, reliable and durable hardware, all while performing well in Moon-like conditions like reduced gravity and complex terrain.”

The total prize purse is $1.5 million, with the first-place winner taking home $1 million and the second-place winner receiving $500,000.

The Break the Ice Lunar Challenge is a NASA Centennial Challenge led by Marshall, with support from NASA’s Kennedy Space Center. Centennial Challenges are part of the Prizes, Challenges, and Crowdsourcing program under NASA’s Space Technology Mission Directorate. Ensemble Consultancy supports challenge competitors.

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

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Mars, Venus Appear Very Close to Each Other this Month

By Lauren Perkins

February is a great month for the early rising skygazers. Venus has been bright in the morning sky all year, rising just before the Moon.

This graphic shows Venus, Earth and its Moon, and Mars.
This graphic shows Venus, Earth and its Moon, and Mars.
NASA/JPL-Caltech/ESA

In the minutes before dawn this week, Venus will rise to the upper left of the waning crescent Moon and will be joined by Mars. Over the coming weeks, Venus will shift towards Mars until they appear to merge into one another, just a half a degree apart, on Feb. 22.

To view this planetary illusion, you’ll need to find a place with a clear view of the western horizon – few to no tall trees or buildings.

For more skygazing opportunities, including observing spiral galaxy M81, check out the video from Jet Propulsion Laboratory’s monthly “What’s Up” video series.

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

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      The suspected IMBH reached maximum brightness in 2012 and then continued declining to 2023. The optical and X-ray observations over the period do not overlap, so this complicates the interpretation. The black hole may have ripped apart a captured star, creating a plasma disk that displays variability, or it may have formed a disk that flickers as gas plummets toward the black hole.
      “If the IMBH is eating a star, how long does it take to swallow the star’s gas? In 2009, HLX-1 was fairly bright. Then in 2012, it was about 100 times brighter. And then it went down again,” said study co-author Roberto Soria of the Italian National Institute for Astrophysics (INAF). “So now we need to wait and see if it’s flaring multiple times, or there was a beginning, there was peak, and now it’s just going to go down all the way until it disappears.”
      The IMBH is on the outskirts of the host galaxy, NGC 6099, about 40,000 light-years from the galaxy’s center. There is presumably a supermassive black hole at the galaxy’s core, which is currently quiescent and not devouring a star.
      Black Hole Building Blocks
      The team emphasizes that doing a survey of IMBHs can reveal how the larger supermassive black holes form in the first place. There are two alternative theories. One is that IMBHs are the seeds for building up even larger black holes by coalescing together, since big galaxies grow by taking in smaller galaxies. The black hole in the middle of a galaxy grows as well during these mergers. Hubble observations uncovered a proportional relationship: the more massive the galaxy, the bigger the black hole. The emerging picture with this new discovery is that galaxies could have “satellite IMBHs” that orbit in a galaxy’s halo but don’t always fall to the center.
      Another theory is that the gas clouds in the middle of dark-matter halos in the early universe don’t make stars first, but just collapse directly into a supermassive black hole. NASA’s James Webb Space Telescope’s discovery of very distant black holes being disproportionately more massive relative to their host galaxy tends to support this idea.
      However, there could be an observational bias toward the detection of extremely massive black holes in the distant universe, because those of smaller size are too faint to be seen. In reality, there could be more variety out there in how our dynamic universe constructs black holes. Supermassive black holes collapsing inside dark-matter halos might simply grow in a different way from those living in dwarf galaxies where black-hole accretion might be the favored growth mechanism.
      “So if we are lucky, we’re going to find more free-floating black holes suddenly becoming X-ray bright because of a tidal disruption event. If we can do a statistical study, this will tell us how many of these IMBHs there are, how often they disrupt a star, how bigger galaxies have grown by assembling smaller galaxies.” said Soria.
      The challenge is that Chandra and XMM-Newton only look at a small fraction of the sky, so they don’t often find new tidal disruption events, in which black holes are consuming stars. The Vera C. Rubin Observatory in Chile, an all-sky survey telescope from the U.S. National Science Foundation and the Department of Energy, could detect these events in optical light as far as hundreds of millions of light-years away. Follow-up observations with Hubble and Webb can reveal the star cluster around the black hole.
      The Hubble Space Telescope has been operating for more than three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.
      Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Related Images & Videos
      NGC 6099 (Hubble + Chandra)
      A Hubble Space Telescope image of a pair of galaxies: NGC 6099 (lower left) and NGC 6098 (upper right). The purple blob depicts X-ray emission from a compact star cluster. The X-rays are produced by an intermediate-mass black hole tearing apart a star.


      NGC 6099 (Hubble)
      A Hubble Space Telescope image of a pair of galaxies: NGC 6099 (lower left) and NGC 6098 (upper right). The white dot labeled HLX-1 is the visible-light component of the location of a compact star cluster where an intermediate-mass black hole is tearing apart a star.


      NGC 6099 Compass Image
      This compass image shows two elliptical galaxies, NGC 6098 at upper right and NGC 6099 at lower left. The fuzzy purple blob at bottom center shows X-ray emission produced by an intermediate-mass black hole tearing apart a star. 


      HLX-1 Illustration
      This sequence of artistic illustrations, from upper left to bottom right, shows how a black hole in the core of a star cluster captures a bypassing star and gravitationally shreds it until there is an explosion, seen in the outskirts of the host galaxy.


      HLX-1 Animation
      This video is an illustration of an intermediate-mass black hole capturing and gravitationally shredding a star. It begins by zooming into a pair of galaxies. The galaxy at lower left, NGC 6099, contain a dense star cluster at center. The video then zooms into the heart of the cl…




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      Last Updated Jul 24, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Contact Media Claire Andreoli
      NASA’s Goddard Space Flight Center
      Greenbelt, Maryland
      claire.andreoli@nasa.gov
      Ray Villard
      Space Telescope Science Institute
      Baltimore, Maryland
      Related Terms
      Hubble Space Telescope Astrophysics Astrophysics Division Black Holes Chandra X-Ray Observatory Galaxies Goddard Space Flight Center Marshall Astrophysics Marshall Space Flight Center
      Related Links and Documents
      Chinese translation of release Science Paper: Multiwavelength Study of a Hyperluminous X-Ray Source near NGC6099: A Strong IMBH Candidate, PDF (1.81 MB)

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      An image of Betelgeuse, the yellow-red star, and the signature of its close companion, the faint blue object.Data: NASA/JPL/NOIRlab. Visualization: NOIRLAB. A century-old hypothesis that Betelgeuse, the 10th brightest star in our night sky, is orbited by a very close companion star was proved true by a team of astrophysicists led by a scientist at NASA’s Ames Research Center in California’s Silicon Valley.
      The research published in The Astrophysical Journal Letters in the paper “Probable Direct Imaging Discovery of the Stellar Companion to Betelgeuse.”
      Fluctuations in the brightness and measured velocity of Betelgeuse, the closest red supergiant star to Earth, had long presented clues that it may have a partner, but the bigger star’s intense glow made direct observations of any fainter neighbors nearly impossible.
      Two recent studies by other teams of astronomers reignited the companion star hypothesis by using more than 100 years of Betelgeuse observations to provide predictions of the companion’s location and brightness.
      If the smaller star did exist, the location predictions suggested that scientists had a window of just a few months to observe the companion star at its widest separation from Betelgeuse, as it orbited near the visible edge of the supergiant. After that, they would have to wait another three years for it to orbit to the other side and again leave the overpowering glow of its larger companion.
      Searches for the companion were initially made using space-based telescopes, because observing through Earth’s atmosphere can blur images of astronomical objects. But these efforts did not detect the companion.
      Steve Howell, a senior research scientist at Ames, recognized the ground-based Gemini North telescope in Hawai’i, one of the largest in the world, paired with a special, high-resolution camera built by NASA, had the potential to directly observe the close companion to Betelgeuse, despite the atmospheric blurring.
      Officially called the ‘Alopeke speckle instrument, the advanced imaging camera let them obtain many thousands of short exposures to measure the atmospheric interference in their data and remove it with detailed image processing, providing an image of Betelgeuse and its companion.
      Howell’s team detected the very faint companion star right where it was predicted to be, orbiting very close to the outer edge of Betelgeuse.
      “I hope our discovery excites other astrophysicists about the robust power of ground-based telescopes and speckle imagers – a key to opening new observational windows,” said Howell. “This can help unlock the great mysteries in our universe.”
      To start, this discovery of a close companion to Betelgeuse may explain why other similar red supergiant stars undergo periodic changes in their brightness on the scale of many years.
      Howell plans to continue observations of Betelgeuse’s stellar companion to better understand its nature. The companion star will again return to its greatest separation from Betelgeuse in November 2027, a time when it will be easiest to detect.
      Having found the long-anticipated companion star, Howell turned to giving it a name. The traditional star name “Betelgeuse” derives from Arabic, meaning “the hand of al-Jawza’,” a female figure in old Arabian legend. Fittingly, Howell’s team named the orbiting companion “Siwarha,” meaning “her bracelet.”
      Photo of the constellation Orion, showing the location of Betelgeuse – and its newfound companion star.NOIRLab/Eckhard Slawik The NASA–National Science Foundation Exoplanet Observational Research Program (NN-EXPLORE) is a joint initiative to advance U.S. exoplanet science by providing the community with access to cutting-edge, ground-based observational facilities. Managed by NASA’s Exoplanet Exploration Program, NN-EXPLORE supports and enhances the scientific return of space missions such as Kepler, TESS (Transiting Exoplanet Survey Satellite), Hubble Space Telescope, and James Webb Space Telescope by enabling essential follow-up observations from the ground—creating strong synergies between space-based discoveries and ground-based characterization. NASA’s Exoplanet Exploration Program is located at the agency’s Jet Propulsion Laboratory.
      To learn more about NN-EXPLORE, visit:
      https://exoplanets.nasa.gov/exep/NNExplore/overview
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      Last Updated Jul 23, 2025 Related Terms
      Astrophysics Ames Research Center Ames Research Center's Science Directorate Astrophysics Division Exoplanet Exploration Program General Science & Research Science Mission Directorate Explore More
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