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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.

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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.

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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.

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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.

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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)

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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.

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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.”

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      This image itself was also the final work of one of Hubble’s instruments: the Wide Field and Planetary Camera 2 (WFPC2). Installed in 1993 to replace the original Wide Field and Planetary Camera, WFPC2 was responsible for some of Hubble’s most enduring images and fascinating discoveries. Hubble’s Wide Field Camera 3 replaced WFPC2 in 2009, during Hubble’s final servicing mission. A mere ten days before astronauts removed Hubble’s WFPC2 from the telescope, the instrument collected the data used in this image: a fitting send-off after 16 years of discoveries. Image processors used the latest and most advanced processing techniques to bring the data to life one more time, producing this breathtaking new view of Kohoutek 4-55.
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      Last Updated Apr 10, 2025 Editor Andrea Gianopoulos Location NASA Goddard Space Flight Center Related Terms
      Hubble Space Telescope Astrophysics Astrophysics Division Emission Nebulae Goddard Space Flight Center Nebulae Planetary Nebulae Stars The Universe Keep Exploring Discover More Topics From Hubble
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    • 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 6 Min Read NASA Webb’s Autopsy of Planet Swallowed by Star Yields Surprise
      NASA’s James Webb Space Telescope’s observations of what is thought to be the first-ever recorded planetary engulfment event revealed a hot accretion disk surrounding the star, with an expanding cloud of cooler dust enveloping the scene. Webb also revealed that the star did not swell to swallow the planet, but the planet’s orbit actually slowly depreciated over time, as seen in this artist’s concept. Full illustration below. Credits:
      NASA, ESA, CSA, R. Crawford (STScI) Observations from NASA’s James Webb Space Telescope have provided a surprising twist in the narrative surrounding what is believed to be the first star observed in the act of swallowing a planet. The new findings suggest that the star actually did not swell to envelop a planet as previously hypothesized. Instead, Webb’s observations show the planet’s orbit shrank over time, slowly bringing the planet closer to its demise until it was engulfed in full.
      “Because this is such a novel event, we didn’t quite know what to expect when we decided to point this telescope in its direction,” said Ryan Lau, lead author of the new paper and astronomer at NSF NOIRLab (National Science Foundation National Optical-Infrared Astronomy Research Laboratory) in Tuscon, Arizona. “With its high-resolution look in the infrared, we are learning valuable insights about the final fates of planetary systems, possibly including our own.”
      Two instruments aboard Webb conducted the post-mortem of the scene – Webb’s MIRI (Mid-Infrared Instrument) and NIRSpec (Near-Infrared Spectrograph). The researchers were able to come to their conclusion using a two-pronged investigative approach.
      Image A: Planetary Engulfment Illustration
      NASA’s James Webb Space Telescope’s observations of what is thought to be the first-ever recorded planetary engulfment event revealed a hot accretion disk surrounding the star, with an expanding cloud of cooler dust enveloping the scene. Webb also revealed that the star did not swell to swallow the planet, but the planet’s orbit actually slowly depreciated over time, as seen in this artist’s concept. NASA, ESA, CSA, R. Crawford (STScI) Constraining the How
      The star at the center of this scene is located in the Milky Way galaxy about 12,000 light-years away from Earth.
      The brightening event, formally called ZTF SLRN-2020, was originally spotted as a flash of optical light using the Zwicky Transient Facility at the Palomar Observatory in San Diego, California. Data from NASA’s NEOWISE (Near-Earth Object Wide-field Infrared Survey Explorer) showed the star actually brightened in the infrared a year before the optical light flash, hinting at the presence of dust. This initial 2023 investigation led researchers to believe that the star was more Sun-like, and had been in the process of aging into a red giant over hundreds of thousands of years, slowly expanding as it exhausted its hydrogen fuel.
      However, Webb’s MIRI told a different story. With powerful sensitivity and spatial resolution, Webb was able to precisely measure the hidden emission from the star and its immediate surroundings, which lie in a very crowded region of space. The researchers found the star was not as bright as it should have been if it had evolved into a red giant, indicating there was no swelling to engulf the planet as once thought.
      Reconstructing the Scene
      Researchers suggest that, at one point, the planet was about Jupiter-sized, but orbited quite close to the star, even closer than Mercury’s orbit around our Sun. Over millions of years, the planet orbited closer and closer to the star, leading to the catastrophic consequence.
      “The planet eventually started to graze the star’s atmosphere. Then it was a runaway process of falling in faster from that moment,” said team member Morgan MacLeod of the Harvard-Smithsonian Center for Astrophysics and the Massachusetts Institute of Technology in Cambridge, Massachusetts. “The planet, as it’s falling in, started to sort of smear around the star.”
      In its final splashdown, the planet would have blasted gas away from the outer layers of the star. As it expanded and cooled off, the heavy elements in this gas condensed into cold dust over the next year.
      Inspecting the Leftovers
      While the researchers did expect an expanding cloud of cooler dust around the star, a look with the powerful NIRSpec revealed a hot circumstellar disk of molecular gas closer in. Furthermore, Webb’s high spectral resolution was able to detect certain molecules in this accretion disk, including carbon monoxide.
      “With such a transformative telescope like Webb, it was hard for me to have any expectations of what we’d find in the immediate surroundings of the star,” said Colette Salyk of Vassar College in Poughkeepsie, New York, an exoplanet researcher and co-author on the new paper. “I will say, I could not have expected seeing what has the characteristics of a planet-forming region, even though planets are not forming here, in the aftermath of an engulfment.”
      The ability to characterize this gas opens more questions for researchers about what actually happened once the planet was fully swallowed by the star.
      “This is truly the precipice of studying these events. This is the only one we’ve observed in action, and this is the best detection of the aftermath after things have settled back down,” Lau said. “We hope this is just the start of our sample.”
      These observations, taken under Guaranteed Time Observation program 1240, which was specifically designed to investigate a family of mysterious, sudden, infrared brightening events, were among the first Target of Opportunity programs performed by Webb. These types of study are reserved for events, like supernova explosions, that are expected to occur, but researchers don’t exactly know when or where. NASA’s space telescopes are part of a growing, international network that stands ready to witness these fleeting changes, to help us understand how the universe works.
      Researchers expect to add to their sample and identify future events like this using the upcoming Vera C. Rubin Observatory and NASA’s Nancy Grace Roman Space Telescope, which will survey large areas of the sky repeatedly to look for changes over time.
      The team’s findings appear today in The Astrophysical Journal.
      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).
      To learn more about Webb, visit: https://science.nasa.gov/webb
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      Media Contacts
      Laura Betz – laura.e.betz@nasa.gov
      NASA’s Goddard Space Flight Center, Greenbelt, Md.
      Hannah Braun – hbraun@stsci.edu
      Space Telescope Science Institute, Baltimore, Md.
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      Last Updated Apr 10, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms
      James Webb Space Telescope (JWST) Astrophysics Exoplanets Goddard Space Flight Center Science & Research Stars The Milky Way The Universe 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 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
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      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
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