Jump to content

Recommended Posts

  • Publishers
Posted
15 Min Read

The Marshall Star for July 10, 2024

The Artemis II Core Stage moves from final assembly to the VAB at NASA’s Michoud Assembly Facility in New Orleans in preparation for delivery to Kennedy Spaceflight Center later this month. Image credit: NASA/Michael DeMocker

NASA Moon Rocket Stage for Artemis II Moved, Prepped for Shipment

NASA is preparing the SLS (Space Launch System) rocket core stage that will help power the first crewed mission of NASA’s Artemis campaign for shipment. On July 6, NASA and Boeing, the core stage lead contractor, moved the Artemis II rocket stage to another part of the agency’s Michoud Assembly Facility. The move comes as teams prepare to roll the massive rocket stage to the agency’s Pegasus barge for delivery to NASA’s Kennedy Space Center in mid-July.

The Artemis II Core Stage moves from final assembly to the VAB at NASA’s Michoud Assembly Facility in New Orleans in preparation for delivery to Kennedy Spaceflight Center later this month. Image credit: NASA/Michael DeMocker
On July 6, NASA and Boeing, the core stage lead contractor, move the Artemis II rocket stage at the agency’s Michoud Assembly Facility. The move comes as teams prepare to roll the massive rocket stage to the agency’s Pegasus barge for delivery to NASA’s Kennedy Space Center in mid-July.
NASA/Michael DeMocker

Prior to the move, technicians began removing external access stands, or scaffolding, surrounding the rocket stage in early June. NASA and Boeing teams used the scaffolding surrounding the core stage to assess the interior elements, including its complex avionics and propulsion systems. The 212-foot core stage has two huge propellant tanks, avionics and flight computer systems, and four RS-25 engines, which together enable the stage to operate during launch and flight.

The stage is fully manufactured and assembled at Michoud. Building, assembling, and transporting is a joint process for NASA, Boeing, and lead RS-25 engines contractor Aerojet Rocketdyne, an L3Harris Technologies company.

Teams at NASA’s Michoud Assembly Facility are preparing the core stage of the agency’s SLS (Space Launch System) for shipment to the agency’s Kennedy Space Center. The 212-foot-tall core stage and its four RS-25 engines will help power Artemis II, the first crewed mission of NASA’s Artemis campaign. In this video, watch as crew remove the external access stands, or scaffolding, before moving the rocket hardware to another area of the facility. (NASA)

NASA is working to land the first woman, first person of color, and its first international partner astronaut on the Moon under Artemis. SLS is part of NASA’s backbone for deep space exploration, along with the Orion spacecraft, supporting ground systems, 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 launch.

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

› Back to Top

Marshall Researchers Battle Biofilm in Space

By Rick Smith

A small group of scientists on the biofilm mitigation team at NASA’s Marshall Space Center study solutions to combat fast-growing colonies of bacteria or fungi, known as biofilm, for future space missions.

Biofilm occurs when a cluster of bacteria or fungi generates a slimy matrix of “extracellular polymeric substances” to protect itself from adverse environmental factors. Biofilm can be found nearly anywhere, from the gray-green scum floating on stagnant pond water to the pinkish ring of residue in a dirty bathtub.

An interconnected series of compact bioreactors, each a cylinder roughly the size of a Thermos with a network of tubing, sensors, and gauges whereby NASA scientists can monitor and measure biofilm growth as each canister’s temperature, filters, and other factors are changed. The biofilm test rack is housed in a laboratory at NASA’s Marshall Space Flight Center in Huntsville, Alabama.
The biofilm mitigation research team at NASA’s Marshall Space Flight Center assembled its own test stand to undertake a multi-month assessment of a variety of natural and chemical compounds and strategies for eradicating biofilm accretion caused by bacteria and fungi in the wastewater tank assembly on the International Space Station. Testing will help NASA extend the lifecycle of water reclamation and recycling hardware and ensure astronauts can sustain clean, healthy water supplies on long-duration missions in space and on other worlds.
NASA/Eric Beitle

For medical, food production, and wastewater processing industries, biofilm is often a costly issue. But offworld, biofilm proves to be even more resilient.

“Bacteria shrug off many of the challenges humans deal with in space, including microgravity, pressure changes, ultraviolet light, nutrient levels, even radiation,” said Yo-Ann Velez-Justiniano, a Marshall microbiologist and environmental control systems engineer.

“Biofilm is icky, sticky – and hard to kill,” said Liezel Koellner, a chemical engineer and NASA Pathways intern from North Carolina State University in Raleigh. Koellner used sophisticated epifluorescence microscopy, 3D visualizations of 2D images captured at different focal planes, to fine-tune the team’s studies.

Keenly aware of the potential hurdles biofilm could pose in future Artemis-era spacecraft and lunar habitats, NASA tasked engineers and chemists at Marshall to study mitigation techniques. Marshall built and maintains the International Space Station’s ECLSS (Environment Control and Life Support System) and is developing next-generation air and water reclamation and recycling technologies, including the system’s wastewater tank assembly.

“The wastewater tank is ‘upstream’ from most of our built-in water purification methods. Because it’s a wastewater feed tank, bacteria and fungus grow well there, generating enough biofilm to clog flow paths and pipes along the route,” said Eric Beitle, ECLSS test engineer at Marshall.

To date, the solution has been to pull and replace old hardware once parts become choked with biofilm. But engineers want to avoid the need for such tactics.

“Even with the ability to 3D-print spare parts on the Moon or Mars, it makes sense to find strategies that prevent biofilm buildup in the first place,” said Velez-Justiniano.

The team took the first step in June 2023 by publishing the complete genome sequence of several strains of bacteria isolated from the space station’s water reclamation system, all of which cultivate biofilm formation.

A woman, seated, and a man, standing alongside her, both in lab coats, analyze biofilm samples taken from the test rack at NASA’s Marshall Space Flight Center in Huntsville, Alabama.
Yo-Ann Velez-Justiniano, left, and Connor Murphy, right, both Environmental Control and Life Support Systems engineers at Marshall, prepare slides for study of cultured bacterial biofilm in the center’s test facility.
NASA/Eric Beitle

They next designed a test stand simulating conditions in the wastewater tank about 250 miles overhead, which permits simultaneous study of multiple mitigation options. The rig housed eight Centers for Disease Control and Prevention biofilm reactors – cylindrical devices roughly the size of a runner’s water bottle – each 1/60th the size of the actual tank.

Each bioreactor holds up to 21 unique test samples on slides, bathed continuously in a flow of real or ersatz wastewater, timed and measured by the automated system, and closely monitored by the team. Because of the compact bioreactor size, the test stand required 2.1 gallons of ersatz flow per week, continuously trickling 0.1 milliliters per minute into each of the eight bioreactors.

“Essentially, we built a collection of tiny systems that all had to permit minute changes to temperature and pressure, maintain a sterile environment, provide autoclave functionality, and run in harmony for weeks at a time with minimal human intervention,” Beitle said. “One phase of the test series ran nonstop for 65 days, and another lasted 77 days. It was a unique challenge from an engineering perspective.”

Different surface mitigation strategies, upstream counteragents, antimicrobial coatings, and temperature levels were introduced in each bioreactor. One promising test involved duckweed, a plant already recognized as a natural water purification system and for its ability to capture toxins and control wastewater odor. By devouring nutrients upstream of the bioreactor, the duckweed denied the bacteria what it needs to thrive, reducing biofilm growth by up to 99.9%.

Over the course of the three-month testing period, teams removed samples from each bioreactor at regular intervals and prepared for study under a microscope to make a detailed count of the biofilm colony-forming units on each plate.

“Bacteria and fungi are smart,” Velez-Justiniano said. “They adapt. We recognize that it’s going to take a mix of effective biofilm mitigation methods to overcome this challenge.”

Biofilm poses as an obstacle to long-duration spaceflight and extended missions on other worlds where replacement parts may be costly or difficult to obtain. The biofilm mitigation team continues to assess and publish findings, alongside academic and industry partners, and will further their research with a full-scale tank experiment at Marshall. They hope to progress to flight tests, experimenting with various mitigation methods in real microgravity conditions in orbit to find solutions to keep surfaces clean, water potable, and future explorers healthy.

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

› Back to Top

Pathways Intern Liezel Koellner Aids NASA Biofilm Mitigation

By Rick Smith

Liezel Koellner is a NASA Pathways intern pursuing her master’s degree in chemical engineering from North Carolina State University in Raleigh. Like most ambitious young engineers, she sought a variety of different internships to augment her classwork.

But once she got word she’d been chosen to spend the spring 2024 term conducting biochemistry experiments at NASA’s Marshall Space Flight Center, her choice was made.

NASA Pathways intern Liezel Koellner, right, and her mentor Yo-Ann Velez-Justiniano, a microbiologist at NASA’s Marshall Space Flight Center, prepare compact bioreactors to be installed in the Marshall biofilm mitigation test stand, which is helping researchers study ways to curtail bacterial and fungal biofilm growth in water reclamation systems such as the one on the International Space Station.
NASA Pathways intern Liezel Koellner, right, and her mentor Yo-Ann Velez-Justiniano, a microbiologist at NASA’s Marshall Space Flight Center, prepare compact bioreactors to be installed in the Marshall biofilm mitigation test stand, which is helping researchers study ways to curtail bacterial and fungal biofilm growth in water reclamation systems such as the one on the International Space Station.
NASA/Eric Beitle

“As a kid, I never imagined I could work at NASA,” she said. “It was a mind-blowing idea!”

That’s how she wound up spending the semester up to her safety gloves in bacterial goo – helping NASA’s biofilm mitigation team study strategies for vanquishing a pervasive, slimy invader playing havoc with space-based hardware. And Koellner couldn’t be happier.

Biofilm is the sticky goo generated by bacteria or fungi to armor itself against radiation, airlessness, and other conditions in space. Astronauts keep their environment fairly ship-shape – but inside closed water reclamation systems, like the one on the International Space Station, biofilm can thrive, wreaking havoc on critical life support systems.

Joining a team of Marshall microbiologists, chemists, and hardware engineers, Koellner spent weeks cultivating sample bacteria – either simulated stuff chemically created onsite or samples shipped frozen from NASA and Boeing archives. She closely monitored ongoing tests, regularly pulling samples to count biofilm colonies.

Most importantly, she oversaw the use of precision epifluorescence microscopy, which employs 3D visualizations to identify layered growth in 2D sample images. That contribution most impressed Marshall microbiologist Yo-Ann Velez-Justiniano, Koellner’s supervisor and project mentor, who said it dramatically improved data accuracy.

“Liezel was able to more accurately analyze patterns of sample growth and deliver precise quantitative data identifying biofilm progression,” Velez-Justiniano said.

A formula for success

Koellner said she’s always been driven to soak up as much practical experience as possible. She was born in Guam to Filipino parents who later emigrated to San Diego, California, to raise their family. From a young age, she took school very seriously.

Velez-Justiniano, left, who heads the biofilm mitigation science team at Marshall, looks on as Koellner, right, shows off her latest sample findings.
Velez-Justiniano, left, who heads the biofilm mitigation science team at Marshall, looks on as Koellner, right, shows off her latest sample findings.
NASA/Eric Beitle

“I always enjoyed chemistry, observing scientific processes and documenting the effects,” Koellner said, but she was daunted by the challenges of calculus-based physics, used to model systems where change occurs and an integral part of scientific fields serving space exploration, engineering, pharmacology, and more.

That changed when she got to the University of North Carolina in Wilmington. “Suddenly, everything clicked,” she said. “With physics, it was amazing to see how math could be applied to real-life applications.”

That practical blend of disciplines led her to consider a career in chemical engineering – using chemical processes to develop products and resources for commercial uses. After completing her bachelor’s degree in chemistry at the University of North Carolina in 2022 and spending a year as a chemist for a private lab in Wilmington, she enrolled at North Carolina State, where she expects to graduate in 2026 with a master’s in chemical engineering.

From water reclamation to air recycling

With the biofilm mitigation tests completed – but her internship continuing until August – Koellner has shifted tracks, moving from the challenges of water reclamation to oxygen recovery solutions for future space habitats and on other worlds.

She’s part of a different team of Marshall ECLSS (Environment Control and Life Support System) specialists, studying ways to recover oxygen from methane gas. That capability could support a variety of oxygen recovery and recycling systems, saving and storing breathable air instead of just jettisoning it into space along with waste gas products. Koellner will write documentation and help monitor and operate the active test stand, once again working alongside Marshall specialists from various disciplines.

She said their commitment has left a lasting impression.

“Everyone is so willing to lend their expertise to pursue work that could impact NASA missions years or even decades in the future,” she said. “The diligence and enthusiasm here are tangible things. That’s the kind of engineer – the kind of person – I want to be.”

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

› Back to Top

Lisa Bates Named Director of Marshall’s Engineering Directorate

Lisa Bates has been named director of the Engineering Directorate at NASA’s Marshall Space Flight Center, effective July 14. In her new role, Bates will be responsible for the center’s largest organization, comprised of more than 2,500 civil service and contractor personnel, who design, test, evaluate, and operate flight hardware and software associated with Marshall-developed space transportation and spacecraft systems, science instruments, and payloads.

Lisa Bates
Lisa Bates has been named director of the Engineering Directorate at NASA’s Marshall Space Flight Center.
NASA

Since November 2023, Bates has served as deputy director of the Engineering Directorate. She was also previously director of Marshall’s Test Laboratory. Appointed to the position in 2021, Bates provided executive leadership for all aspects of the Laboratory, including workforce, budget, infrastructure, and operations for testing.

She joined Marshall in 2008 as the Ares I Upper Stage Thrust Vector Control lead in the Propulsion Department. Since then, she has served in positions of increasing responsibility and authority. From 2009 to 2017, she served as the first chief of the new TVC Branch, which was responsible for defining operational requirements, performing analysis, and evaluating Launch Vehicle TVC systems and TVC components.

As the Space Launch System (SLS) Program Executive from 2017 to 2018, Bates supported the NASA Deputy Associate Administrator for Exploration Systems Development as the liaison and advocate of the SLS. Upon returning to MSFC in 2018, she was selected as deputy manager of the SLS Booster Element Office. Bates also served as deputy manager of the SLS Stages Office from 2018 to 2021 where she shared the responsibilities, accountability, and authorities for all activities associated with the requirements definition, design, development, manufacturing, assembly, green run test, and delivery of the SLS Program’s Stages Element.

Prior to her NASA career, Bates worked 18 years in private industry for numerous aerospace and defense contractors, including Jacobs Engineering, Marotta Scientific Controls, United Technologies (USBI), United Defense, and Sverdrup Technologies.

Bates holds a bachelor’s degree in mechanical engineering from the University of Alabama in Huntsville. She was awarded a NASA Outstanding Leadership Medal in 2013 and 2022 and has received numerous group and individual achievement awards.

› Back to Top

Orion on the Rise

The Artemis II Orion spacecraft is pictured surrounded by the metal walls of the altitude chamber. Orion is a cone shaped spacecraft with metal and wires exposed. Technicians stand around the open top of the altitude chamber.

Technicians lift NASA’s Orion spacecraft out of the Final Assembly and System Testing cell at NASA’s Kennedy Space Center on June 28. The integrated spacecraft, which will be used for the Artemis II mission to orbit the Moon, has been undergoing final rounds of testing and assembly, including end-to-end performance verification of its subsystems and checking for leaks in its propulsion systems. A 30-ton crane returned Orion into the recently renovated altitude chamber where it underwent electromagnetic testing. The spacecraft now will undergo a series of tests that will subject it to a near-vacuum environment by removing air, thus creating a space where the pressure is extremely low. This results in no atmosphere, similar to the one the spacecraft will experience during future lunar missions. The data recorded during these tests will be used to qualify the spacecraft to safely fly the Artemis II astronauts through the harsh environment of space. (NASA/Radislav Sinyak)

› Back to Top

NASA to Cover Northrop Grumman’s 20th Cargo Space Station Departure

Northrop Grumman’s uncrewed Cygnus spacecraft is scheduled to depart the International Space Station on July 12, five and a half months after delivering more than 8,200 pounds of supplies, scientific investigations, commercial products, hardware, and other cargo to the orbiting laboratory for NASA and its international partners.

53754025187-238e5065da-k.jpg?w=2047
Northrop Grumman’s Cygnus spacecraft and the International Space Station above western Mongolia.
NASA

This mission was the company’s 20th commercial resupply mission to the space station for NASA.

Live coverage of the spacecraft’s departure will begin at 5:30 a.m. CDT on the NASA+, NASA Television, the NASA app, YouTube, and the agency’s website. Learn how to stream NASA TV through a variety of platforms including social media.

Flight controllers on the ground will send commands for the space station’s Canadarm2 robotic arm to detach Cygnus from the Unity module’s Earth-facing port, then maneuver the spacecraft into position for its release at 6 a.m. NASA astronaut Mike Barratt will monitor Cygnus’ systems upon its departure from the space station.

Following unberthing, the Kentucky Re-entry Probe Experiment-2 (KREPE-2), stowed inside Cygnus, will take measurements to demonstrate a thermal protection system for the spacecraft and its contents during re-entry in Earth’s atmosphere.

Cygnus – filled with trash packed by the station crew – will be commanded to deorbit July 13, setting up a destructive re-entry in which the spacecraft will safely burn up in Earth’s atmosphere.

The Northrop Grumman spacecraft arrived at the space station Feb. 1, following a launch on a SpaceX Falcon 9 rocket from Space Launch Complex 40 at Cape Canaveral Space Force Station.

The HOSC (Huntsville Operations Support Center) at NASA’s Marshall Space Flight Center provides engineering and mission operations support for the space station, the Commercial Crew Program, and Artemis missions, as well as science and technology demonstration missions. The Payload Operations Integration Center within the HOSC operates, plans, and coordinates the science experiments onboard the space station 365 days a year, 24 hours a day.

Get breaking news, images, and features from the space station on the station blog.

› Back to Top

Happy Birthday, Meatball! NASA’s Iconic Logo Turns 65

On July 15, NASA’s logo is turning 65. The iconic symbol, known affectionately as “the meatball,” was developed at NASA’s Lewis Research Center (now called NASA Glenn). Employee James Modarelli, who started his career at the center as an artist and technical illustrator, was its chief designer.

A painter stands in the bucket of a crane lift and reaches out to apply a fresh coat of paint to the red, white, and blue NASA logo painted on a tan, corrugated hangar façade. He is holding a paint brush and a can of paint and wearing a harness, blue jeans, a white shirt, and sunglasses.
A painter applies a fresh coat of paint to the NASA “meatball” logo on the north façade of Glenn Research Center’s Flight Research Building, or hangar, in 2006.
NASA/Marvin Smith

The red, white, and blue design, which includes elements representing NASA’s space and aeronautics missions, became the official logo of the United States’ new space agency in 1959. A simplified version of NASA’s formal seal, the symbol has launched on rockets, flown to the Moon and beyond, and even adorns the International Space Station.

In this black-and-white photo, three workers stand below a large NASA logo sign. Two of the workers hold either end of the sign. They stand in front of a hangar building with scaffolding.
Workers install the NASA “meatball” logo on the front of the Flight Research Building, or hangar, at Lewis Research Center (now NASA Glenn) in 1962.
NASA

Along with its importance as a timeless symbol of exploration and discovery, the logo is also one of the world’s most recognized brand symbols. It gained its nickname in 1975 to differentiate it from NASA’s “worm” logotype. The “meatball” and these other NASA designs have made waves in pop culture.

“NASA’s brand elements are wildly popular,” said Aimee Crane, merchandising and branding clearance manager for the agency. “Every year, the agency receives requests to merchandise more than 10,000 NASA-inspired items.”

› Back to Top

View the full article

Join the conversation

You can post now and register later. If you have an account, sign in now to post with your account.
Note: Your post will require moderator approval before it will be visible.

Guest
Reply to this topic...

×   Pasted as rich text.   Paste as plain text instead

  Only 75 emoji are allowed.

×   Your link has been automatically embedded.   Display as a link instead

×   Your previous content has been restored.   Clear editor

×   You cannot paste images directly. Upload or insert images from URL.

  • Similar Topics

    • 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 Hubble’s Partners in Science Universe Uncovered Explore the Night Sky Observatory Hubble Observatory Hubble Design Mission Operations Missions to Hubble Hubble vs Webb Team Hubble Team Career Aspirations Hubble Astronauts News Hubble News Social Media Media Resources Multimedia Multimedia Images Videos Sonifications Podcasts e-Books Online Activities Lithographs Fact Sheets Posters Hubble on the NASA App Glossary More 35th Anniversary Online Activities 2 min read
      Hubble Studies a Nearby Galaxy’s Star Formation
      This NASA/ESA Hubble Space Telescope image features the picturesque spiral galaxy NGC 4941. ESA/Hubble & NASA, D. Thilker This NASA/ESA Hubble Space Telescope image features the picturesque spiral galaxy NGC 4941, which lies about 67 million light-years from Earth in the constellation Virgo (The Maiden). Because this galaxy is nearby, cosmically speaking, Hubble’s keen instruments are able to pick out exquisite details such as individual star clusters and filamentary clouds of gas and dust.
      The data used to construct this image were collected as part of an observing program that investigates the star formation and stellar feedback cycle in nearby galaxies. As stars form in dense, cold clumps of gas, they begin to influence their surroundings. Stars heat and stir up the gas clouds in which they form through winds, starlight, and — eventually, for massive stars — by exploding as supernovae. These processes are collectively called stellar feedback, and they influence the rate at which a galaxy can form new stars.
      As it turns out, stars aren’t the only entities providing feedback in NGC 4941. At the heart of this galaxy lies an active galactic nucleus: a supermassive black hole feasting on gas. As the black hole amasses gas from its surroundings, the gas swirls into a superheated disk that glows brightly at wavelengths across the electromagnetic spectrum. Similar to stars — but on a much, much larger scale — active galactic nuclei shape their surroundings through winds, radiation, and powerful jets, altering not only star formation but also the evolution of the galaxy as a whole.
      Facebook logo @NASAHubble @NASAHubble Instagram logo @NASAHubble Media Contact:
      Claire Andreoli (claire.andreoli@nasa.gov)
      NASA’s Goddard Space Flight Center, Greenbelt, MD
      Share








      Details
      Last Updated Apr 04, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
      Hubble Space Telescope Astrophysics Astrophysics Division Galaxies Goddard Space Flight Center Spiral Galaxies The Universe Keep Exploring Discover More Topics From Hubble
      Hubble Space Telescope


      Since its 1990 launch, the Hubble Space Telescope has changed our fundamental understanding of the universe.


      Hubble’s Night Sky Challenge



      Hubble’s Galaxies



      35 Years of Hubble Images


      View the full article
    • By European Space Agency
      Image: This image shows Webb’s recent observation of the asteroid 2024 YR4 using both its Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI). Data from NIRCam shows reflected light, while the MIRI observations show thermal light.
      On 8 March 2025, the NASA/ESA/CSA James Webb Space Telescope turned its watchful eye toward asteroid 2024 YR4, which we now know poses no significant threat to Earth in 2032 and beyond.
      This is the smallest object targeted by Webb to date, and one of the smallest objects to have its size directly measured.
      Observations were taken to study the thermal properties of 2024 YR4, including how quickly it heats up and cools down and how hot it is at its current distance from the Sun. These measurements indicate that this asteroid does not share properties observed in larger asteroids. This is likely a combination of its fast spin and lack of fine-grained sand on its surface. Further research is needed, however this is considered consistent with a surface dominated by rocks that are roughly fist-sized or larger.
      Asteroid 2024 YR4 was recently under close watch by the team at ESA's Near Earth Objects Coordination Centre, located in Italy. Planetary defence experts from the Agency's Space Safety programme worked with NASA and the international asteroid community to closely watch this object and refine its orbit, which was eventually determined to not pose a risk of Earth impact. Read details on this unusual campaign via ESA's Rocket Science blog and in news articles here and here.
      Webb’s observations indicate that the asteroid measures roughly 60 meters (comparable to the height of a 15-story building).
      The new observations from Webb not only provide unique information about 2024 YR4’s size, but can also complement ground-based observations of the object's position to help improve our understanding of the object’s orbit and future trajectory.
      Note: This post highlights data from Webb science in progress, which has not yet been through the peer-review process.
      [Image description: A collage of three images showing the black expanse of space. Two-thirds of the collage is taken up by the black background sprinkled with small, blurry galaxies in orange, blue, and white. There are two images in a column at the right side of the collage. On the right side of the main image, not far from the top, a very faint dot is outlined with a white square. At the right, there are two zoomed in views of this area. The top box is labeled NIRCam and shows a fuzzy dot at the center of the inset. The bottom box is labeled MIRI and shows a fuzzy pinkish dot.]
      View the full article
    • By NASA
      Explore This Section Webb News Latest News Latest Images Blog (offsite) Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Observatory Overview Launch Deployment Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning 5 Min Read NASA Webb Explores Effect of Strong Magnetic Fields on Star Formation
      An image of the Milky Way captured by the MeerKAT radio telescope array puts the James Webb Space Telescope’s image of the Sagittarius C region in context. Full image below. Credits:
      NASA, ESA, CSA, STScI, SARAO, Samuel Crowe (UVA), John Bally (CU), Ruben Fedriani (IAA-CSIC), Ian Heywood (Oxford) Follow-up research on a 2023 image of the Sagittarius C stellar nursery in the heart of our Milky Way galaxy, captured by NASA’s James Webb Space Telescope, has revealed ejections from still-forming protostars and insights into the impact of strong magnetic fields on interstellar gas and the life cycle of stars.  
      “A big question in the Central Molecular Zone of our galaxy has been, if there is so much dense gas and cosmic dust here, and we know that stars form in such clouds, why are so few stars born here?” said astrophysicist John Bally of the University of Colorado Boulder, one of the principal investigators. “Now, for the first time, we are seeing directly that strong magnetic fields may play an important role in suppressing star formation, even at small scales.”
      Detailed study of stars in this crowded, dusty region has been limited, but Webb’s advanced near-infrared instruments have allowed astronomers to see through the clouds to study young stars like never before.
      “The extreme environment of the galactic center is a fascinating place to put star formation theories to the test, and the infrared capabilities of NASA’s James Webb Space Telescope provide the opportunity to build on past important observations from ground-based telescopes like ALMA and MeerKAT,” said Samuel Crowe, another principal investigator on the research, a senior undergraduate at the University of Virginia and a 2025 Rhodes Scholar.
      Bally and Crowe each led a paper published in The Astrophysical Journal.
      Image A: Milky Way Center (MeerKAT and Webb)
      An image of the Milky Way captured by the MeerKAT (formerly the Karoo Array Telescope) radio telescope array puts the James Webb Space Telescope’s image of the Sagittarius C region in context. Like a super-long exposure photograph, MeerKAT shows the bubble-like remnants of supernovas that exploded over millennia, capturing the dynamic nature of the Milky Way’s chaotic core. At the center of the MeerKAT image the region surrounding the Milky Way’s supermassive black hole blazes bright. Huge vertical filamentary structures echo those captured on a smaller scale by Webb in Sagittarius C’s blue-green hydrogen cloud. NASA, ESA, CSA, STScI, SARAO, Samuel Crowe (UVA), John Bally (CU), Ruben Fedriani (IAA-CSIC), Ian Heywood (Oxford) Image B: Milky Way Center (MeerKAT and Webb), Labeled
      The star-forming region Sagittarius C, captured by the James Webb Space Telescope, is about 200 light-years from the Milky Way’s central supermassive black hole, Sagittarius A*. The spectral index at the lower left shows how color was assigned to the radio data to create the image. On the negative end, there is non-thermal emission, stimulated by electrons spiraling around magnetic field lines. On the positive side, thermal emission is coming from hot, ionized plasma. For Webb, color is assigned by shifting the infrared spectrum to visible light colors. The shortest infrared wavelengths are bluer, and the longer wavelengths appear more red. NASA, ESA, CSA, STScI, SARAO, Samuel Crowe (UVA), John Bally (CU), Ruben Fedriani (IAA-CSIC), Ian Heywood (Oxford) Using Infrared to Reveal Forming Stars
      In Sagittarius C’s brightest cluster, the researchers confirmed the tentative finding from the Atacama Large Millimeter Array (ALMA) that two massive stars are forming there. Along with infrared data from NASA’s retired Spitzer Space Telescope and SOFIA (Stratospheric Observatory for Infrared Astronomy) mission, as well as the Herschel Space Observatory, they used Webb to determine that each of the massive protostars is already more than 20 times the mass of the Sun. Webb also revealed the bright outflows powered by each protostar.
      Even more challenging is finding low-mass protostars, still shrouded in cocoons of cosmic dust. Researchers compared Webb’s data with ALMA’s past observations to identify five likely low-mass protostar candidates.
      The team also identified 88 features that appear to be shocked hydrogen gas, where material being blasted out in jets from young stars impacts the surrounding gas cloud. Analysis of these features led to the discovery of a new star-forming cloud, distinct from the main Sagittarius C cloud, hosting at least two protostars powering their own jets.
      “Outflows from forming stars in Sagittarius C have been hinted at in past observations, but this is the first time we’ve been able to confirm them in infrared light. It’s very exciting to see, because there is still a lot we don’t know about star formation, especially in the Central Molecular Zone, and it’s so important to how the universe works,” said Crowe.
      Magnetic Fields and Star Formation
      Webb’s 2023 image of Sagittarius C showed dozens of distinctive filaments in a region of hot hydrogen plasma surrounding the main star-forming cloud. New analysis by Bally and his team has led them to hypothesize that the filaments are shaped by magnetic fields, which have also been observed in the past by the ground-based observatories ALMA and MeerKAT (formerly the Karoo Array Telescope).
      “The motion of gas swirling in the extreme tidal forces of the Milky Way’s supermassive black hole, Sagittarius A*, can stretch and amplify the surrounding magnetic fields. Those fields, in turn, are shaping the plasma in Sagittarius C,” said Bally.
      The researchers think that the magnetic forces in the galactic center may be strong enough to keep the plasma from spreading, instead confining it into the concentrated filaments seen in the Webb image. These strong magnetic fields may also resist the gravity that would typically cause dense clouds of gas and dust to collapse and forge stars, explaining Sagittarius C’s lower-than-expected star formation rate. 
      “This is an exciting area for future research, as the influence of strong magnetic fields, in the center of our galaxy or other galaxies, on stellar ecology has not been fully considered,” said Crowe.  
      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 CSA (Canadian Space Agency).
      Downloads
      Click any image to open a larger version.
      View/Download all image products at all resolutions for this article from the Space Telescope Science Institute.
      View/Download the science paper led by Bally from the The Astrophysical Journal.
      View/Download the science paper led by Crowe from the The Astrophysical Journal.
      Media Contacts
      Laura Betz – laura.e.betz@nasa.gov
      NASA’s Goddard Space Flight Center, Greenbelt, Md.
      Leah Ramsay – lramsay@stsci.edu
      Space Telescope Science Institute, Baltimore, Md.
      Christine Pulliam – cpulliam@stsci.edu
      Space Telescope Science Institute, Baltimore, Md.
      Related Information
      Read more: press releases about the center of the Milky Way
      NASA’s Universe of Learning: ViewSpace Interactive image tour of the center of the Milky Way
      Learn more about the Milky Way and Sagittarius Constellation
      More Webb News
      More Webb Images
      Webb Science Themes
      Webb Mission Page
      Related For Kids
      What Is a Nebula?
      What Is a Galaxy?
      What is the Webb Telescope?
      SpacePlace for Kids
      En Español
      ¿Qué es una nebulosa?
      ¿Qué es una galaxia?
      Ciencia de la NASA
      NASA en español 
      Space Place para niños
      Keep Exploring Related Topics
      James Webb Space Telescope


      Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…


      Stars



      Galaxies



      Universe


      Share








      Details
      Last Updated Apr 02, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms
      James Webb Space Telescope (JWST) Astrophysics Galaxies Galaxies, Stars, & Black Holes Goddard Space Flight Center Protostars Science & Research Stars The Milky Way The Universe View the full article
    • By NASA
      X-ray: NASA/CXC/Technion/N. Keshet et al.; Illustration: NASA/CXC/SAO/M. Weiss People often think about archaeology happening deep in jungles or inside ancient pyramids. However, a team of astronomers has shown that they can use stars and the remains they leave behind to conduct a special kind of archaeology in space.
      Mining data from NASA’s Chandra X-ray Observatory, the team of astronomers studied the relics that one star left behind after it exploded. This “supernova archaeology” uncovered important clues about a star that self-destructed – probably more than a million years ago.
      Today, the system called GRO J1655-40 contains a black hole with nearly seven times the mass of the Sun and a star with about half as much mass. However, this was not always the case.
      Originally GRO J1655-40 had two shining stars. The more massive of the two stars, however, burned through all of its nuclear fuel and then exploded in what astronomers call a supernova. The debris from the destroyed star then rained onto the companion star in orbit around it, as shown in the artist’s concept.
      This artist’s impression shows the effects of the collapse and supernova explosion of a massive star. A black hole (right) was formed in the collapse and debris from the supernova explosion is raining down onto a companion star (left), polluting its atmosphere.CXC/SAO/M. Weiss With its outer layers expelled, including some striking its neighbor, the rest of the exploded star collapsed onto itself and formed the black hole that exists today. The separation between the black hole and its companion would have shrunk over time because of energy being lost from the system, mainly through the production of gravitational waves. When the separation became small enough, the black hole, with its strong gravitational pull, began pulling matter from its companion, wrenching back some of the material its exploded parent star originally deposited.
      While most of this material sank into the black hole, a small amount of it fell into a disk that orbits around the black hole. Through the effects of powerful magnetic fields and friction in the disk, material is being sent out into interstellar space in the form of powerful winds.
      This is where the X-ray archaeological hunt enters the story. Astronomers used Chandra to observe the GRO J1655-40 system in 2005 when it was particularly bright in X-rays. Chandra detected signatures of individual elements found in the black hole’s winds by getting detailed spectra – giving X-ray brightness at different wavelengths – embedded in the X-ray light. Some of these elements are highlighted in the spectrum shown in the inset.
      The team of astronomers digging through the Chandra data were able to reconstruct key physical characteristics of the star that exploded from the clues imprinted in the X-ray light by comparing the spectra with computer models of stars that explode as supernovae. They discovered that, based on the amounts of 18 different elements in the wind, the long-gone star destroyed in the supernova was about 25 times the mass of the Sun, and was much richer in elements heavier than helium in comparison with the Sun.
      This analysis paves the way for more supernova archaeology studies using other outbursts of double star systems.
      A paper describing these results titled “Supernova Archaeology with X-Ray Binary Winds: The Case of GRO J1655−40” was published in The Astrophysical Journal in May 2024. The authors of this study are Noa Keshet (Technion — Israel Institute of Technology), Ehud Behar (Technion), and Timothy Kallman (NASA’s Goddard Space Flight Center).
      NASA’s Marshall Space Flight Center in Huntsville, Alabama, 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.
      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 an artist’s rendering of a supernova explosion, inset with a spectrum graph.
      The artist’s illustration features a star and a black hole in a system called GRO J1655-40. Here, the black hole is represented by a black sphere to our upper right of center. The star is represented by a bright yellow sphere to our lower left of center. In this illustration, the artist captures the immensely powerful supernova as a black hole is created from the collapse of a massive star, with an intense burst of blurred beams radiating from the black sphere. The blurred beams of red, orange, and yellow light show debris from the supernova streaking across the entire image in rippling waves. These beams rain debris on the bright yellow star.
      When astronomers used the Chandra X-ray Observatory to observe the system in 2005, they detected signatures of individual elements embedded in the X-ray light. Some of those elements are highlighted in the spectrum graph shown in the inset, positioned at our upper lefthand corner.
      The graph’s vertical axis, on our left, indicates X-ray brightness from 0.0 up to 0.7 in intensity units. The horizontal axis, at the bottom of the graph, indicates Wavelength from 6 to 12 in units of Angstroms. On the graph, a tight zigzagging line begins near the top of the vertical axis, and slopes down toward the far end of the horizontal axis. The sharp dips show wavelengths where the light has been absorbed by different elements, decreasing the X-ray brightness. Some of the elements causing these dips have been labeled, including Silicon, Magnesium, Iron, Nickel, Neon, and Cobalt.
      News Media Contact
      Megan Watzke
      Chandra X-ray Center
      Cambridge, Mass.
      617-496-7998
      mwatzke@cfa.harvard.edu
      Lane Figueroa
      Marshall Space Flight Center, Huntsville, Alabama
      256-544-0034
      lane.e.figueroa@nasa.gov
      View the full article
    • By NASA
      The innovative team of engineers and scientists from NASA, the Johns Hopkins Applied Physics Laboratory in Laurel, Maryland, and more than 40 other partner organizations across the country that created the Parker Solar Probe mission has been awarded the 2024 Robert J. Collier Trophy by the National Aeronautic Association (NAA). This annual award recognizes the most exceptional achievement in aeronautics and astronautics in America with respect to improving the performance, efficiency, and safety of air or space vehicles in the previous year.   
      “Congratulations to the entire Parker Solar Probe team for this well-earned recognition,” said NASA acting Administrator Janet Petro. “This mission’s trailblazing research is rewriting the textbooks on solar science by going to a place no human-made object has ever been and advancing NASA’s efforts to better understand our solar system and the Sun’s influence, with lasting benefits for us all. As the first to touch the Sun and fastest human-made object ever built, Parker Solar Probe is a testament to human ingenuity and discovery.”
      An artist’s concept of NASA’s Parker Solar Probe. NASA On Dec. 24, 2024, Parker Solar Probe made its closest approach to the Sun, passing deep within the Sun’s corona, just 3.8 million miles above the Sun’s surface and at a top speed of close to 430,000 mph, ushering in a new era of scientific discovery and space exploration.
      “This award is a recognition of the unrelenting dedication and hard work of the Parker Solar Probe team. I am so proud of this team and honored to have been a part of it,” said Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters in Washington. “By studying the Sun closer than ever before, we continue to advance our understanding of not only our closest star, but also stars across our universe. Parker Solar Probe’s historic close approaches to the Sun are a testament to the incredible engineering that made this record-breaking journey possible.”
      Three novel aerospace technology advancements were critical to enabling this record performance: The first is the Thermal Protection System, or heat shield, that protects the spacecraft and is built to withstand brutal temperatures as high as 2,500 degrees Fahrenheit. The Thermal Protection System allows Parker’s electronics and instruments to operate close to room temperature.
      Additional Parker innovations included first-of-their-kind actively cooled solar arrays that protect themselves from overexposure to intense solar energy while powering the spacecraft, and a fully autonomous spacecraft system that can manage its own flight behavior, orientation, and configuration for months at a time. Parker has relied upon all of these vital technologies every day since its launch almost seven years ago, in August 2018.
      “I am thrilled for the Parker Solar Probe team on receiving this well-deserved award,” said Joe Westlake, director of the Heliophysics Division at NASA Headquarters. “The new information about the Sun made available through this mission will improve our ability to prepare for space weather events across the solar system, as well as better understand the very star that makes life possible for us on Earth.”
      Parker’s close-up observations of solar events, such as coronal mass ejections and solar particle events, are critical to advancing our understanding of the science of our Sun and the phenomena that drive high-energy space weather events that pose risks to satellites, air travel, astronauts, and even power grids on Earth. Understanding the fundamental physics behind events which drive space weather will enable more reliable predictions and lower astronaut exposure to hazardous radiation during future deep space missions to the Moon and Mars.
      “This amazing team brought to life an incredibly difficult space science mission that had been studied, and determined to be impossible, for more than 60 years. They did so by solving numerous long-standing technology challenges and dramatically advancing our nation’s spaceflight capabilities,” said APL Director Ralph Semmel. “The Collier Trophy is well-earned recognition for this phenomenal group of innovators from NASA, APL, and our industry and research partners from across the nation.”
      First awarded in 1911, the Robert J. Collier Trophy winner is selected by a group of aviation leaders chosen by the NAA. The Collier Trophy is housed in the Smithsonian’s National Air and Space Museum in Washington.
      “Traveling three times closer to the Sun and seven times faster than any spacecraft before, Parker’s technology innovations enabled humanity to reach inside the Sun’s atmosphere for the first time,” said Bobby Braun, head of APL’s Space Exploration Sector. “We are all immensely proud that the Parker Solar Probe team will join a long legacy of prestigious aerospace endeavors that redefined technology and changed history.”
      “The Parker Solar Probe team’s achievement in earning the 2024 Collier is a shining example of determination, genius, and teamwork,” said NAA President and CEO Amy Spowart. “It’s a distinct honor for the NAA to acknowledge and celebrate the remarkable team that turned the impossible into reality.”
      Parker Solar Probe was developed as part of NASA’s Living With a Star program to explore aspects of the Sun-Earth system that directly affect life and society. The Living With a Star program is managed by the agency’s Goddard Space Flight Center in Greenbelt, Maryland, for NASA’s Science Mission Directorate in Washington. The Applied Physics Laboratory designed, built, and operates the spacecraft and manages the mission for NASA.
      By Geoff Brown
      Johns Hopkins University Applied Physics Laboratory
      Share








      Details
      Last Updated Mar 25, 2025 Editor Sarah Frazier Contact Abbey Interrante abbey.a.interrante@nasa.gov Location Goddard Space Flight Center Related Terms
      Heliophysics Goddard Space Flight Center Heliophysics Division Parker Solar Probe (PSP) The Sun Explore More
      5 min read NASA’s Parker Solar Probe Makes History With Closest Pass to Sun


      Article


      3 months ago
      4 min read Final Venus Flyby for NASA’s Parker Solar Probe Queues Closest Sun Pass


      Article


      5 months ago
      11 min read NASA Enters the Solar Atmosphere for the First Time, Bringing New Discoveries
      A major milestone and new results from NASA’s Parker Solar Probe were announced on Dec.…


      Article


      3 years ago
      View the full article
  • Check out these Videos

×
×
  • Create New...