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Vivid Portrait of Interacting Galaxies Marks Webb’s Second Anniversary


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Vivid Portrait of Interacting Galaxies Marks Webb’s Second Anniversary

Arp 142, two interacting galaxies, observed in near- and mid-infrared light. At left is NGC 2937, nicknamed the Egg. Its center is the brighter and whiter. There are six diffraction spikes atop its gauzy blue layers. At right is NGC 2936, nicknamed the Penguin. Its beak-like region points toward and above the Egg. Where the eye would be is a small, opaque yellow spiral. The Penguin’s distorted arms form the bird’s beak, back, and tail. The tail is wide and layered, like a beta fish’s tail. A semi-transparent blue hue traces the Penguin and extends from the galaxy, creating an upside-down U over top of both galaxies. At top right is another galaxy seen from the side, pointing roughly at a 45-degree angle. It is largely light blue. Its length appears approximately as long as the Egg’s height. One foreground star with large, bright blue diffraction spikes appears over top of the galaxy and another near it. The entire black background is filled with tiny, extremely distant galaxies.
Webb’s view of the interacting galaxies of Arp 142 that combines Webb’s NIRCam and MIRI instrument images. Full image below.

Two for two! A duo of interacting galaxies commemorates the second science anniversary of NASA’s James Webb Space Telescope, which takes constant observations, including images and highly detailed data known as spectra. Its operations have led to a “parade” of discoveries by astronomers around the world.

“Since President Biden and Vice President Harris unveiled the first image from the James Webb Space Telescope two years ago, Webb has continued to unlock the mysteries of the universe,” said NASA Administrator Bill Nelson. “With remarkable images from the corners of the cosmos, going back nearly to the beginning of time, Webb’s capabilities are shedding new light on our celestial surroundings and inspiring future generations of scientists, astronomers, and explorers.”

“In just two years, Webb has transformed our view of the universe, enabling the kind of world-class science that drove NASA to make this mission a reality,” said Mark Clampin, director of the Astrophysics Division at NASA Headquarters in Washington. “Webb is providing insights into longstanding mysteries about the early universe and ushering in a new era of studying distant worlds, while returning images that inspire people around the world and posing exciting new questions to answer. It has never been more possible to explore every facet of the universe.”

The telescope’s specialization in capturing infrared light — which is beyond what our own eyes can detect — shows these galaxies, collectively known as Arp 142, locked in a slow cosmic dance. Webb’s observations, which combine near- and mid-infrared light from Webb’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument), respectively, clearly show that they are joined by a haze represented in blue that is a mix of stars and gas, a result of their mingling.

Their ongoing interaction was set in motion between 25 and 75 million years ago, when the Penguin (individually cataloged as NGC 2936) and the Egg (NGC 2937) completed their first pass. They will go on to shimmy and sway, completing several additional loops before merging into a single galaxy hundreds of millions of years from now.

Image A: Interacting Galaxies Arp 142 (NIRCam and MIRI)

Arp 142, two interacting galaxies, observed in near- and mid-infrared light. At left is NGC 2937, nicknamed the Egg. Its center is the brighter and whiter. There are six diffraction spikes atop its gauzy blue layers. At right is NGC 2936, nicknamed the Penguin. Its beak-like region points toward and above the Egg. Where the eye would be is a small, opaque yellow spiral. The Penguin’s distorted arms form the bird’s beak, back, and tail. The tail is wide and layered, like a beta fish’s tail. A semi-transparent blue hue traces the Penguin and extends from the galaxy, creating an upside-down U over top of both galaxies. At top right is another galaxy seen from the side, pointing roughly at a 45-degree angle. It is largely light blue. Its length appears approximately as long as the Egg’s height. One foreground star with large, bright blue diffraction spikes appears over top of the galaxy and another near it. The entire black background is filled with tiny, extremely distant galaxies.
The distorted spiral galaxy at center, the Penguin, and the compact elliptical at left, the Egg, are locked in an active embrace. This near- and mid-infrared image combines data from NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) and MIRI (Mid-Infrared Instrument), and marks the telescope’s second year of science. Webb’s view shows that their interaction is marked by a glow of scattered stars represented in blue. Known jointly as Arp 142, the galaxies made their first pass by one another between 25 and 75 million years ago, causing “fireworks,” or new star formation, in the Penguin. The galaxies are approximately the same mass, which is why one hasn’t consumed the other.

Let’s Dance!

Before their first approach, the Penguin held the shape of a spiral. Today, its galactic center gleams like an eye, its unwound arms now shaping a beak, head, backbone, and fanned-out tail.

Like all spiral galaxies, the Penguin is still very rich in gas and dust. The galaxies’ “dance” gravitationally pulled on the Penguin’s thinner areas of gas and dust, causing them to crash in waves and form stars. Look for those areas in two places: what looks like a fish in its “beak” and the “feathers” in its “tail.”

Surrounding these newer stars is smoke-like material that includes carbon-containing molecules, known as polycyclic aromatic hydrocarbons, which Webb is exceptional at detecting. Dust, seen as fainter, deeper orange arcs also swoops from its beak to tail feathers.

In contrast, the Egg’s compact shape remains largely unchanged. As an elliptical galaxy, it is filled with aging stars, and has a lot less gas and dust that can be pulled away to form new stars. If both were spiral galaxies, each would end the first “twist” with new star formation and twirling curls, known as tidal tails.

Another reason for the Egg’s undisturbed appearance: These galaxies have approximately the same mass or heft, which is why the smaller-looking elliptical wasn’t consumed or distorted by the Penguin.

It is estimated that the Penguin and the Egg are about 100,000 light-years apart — quite close in astronomical terms. For context, the Milky Way galaxy and our nearest neighbor, the Andromeda Galaxy, are about 2.5 million light-years apart. They too will interact, but not for about 4 billion years.

Now, look to the top right to spot a galaxy that is not at this party. This edge-on galaxy, cataloged PGC 1237172, is 100 million light-years closer to Earth. It’s also quite young, teeming with new, blue stars.

Want one more party trick? Switch to Webb’s mid-infrared-only image to see PGC 1237172 practically disappear. Mid-infrared light largely captures cooler, older stars and an incredible amount of dust. Since the galaxy’s stellar population is so young, it “vanishes” in mid-infrared light.

Image B: Interacting Galaxies Arp 142 (MIRI Only)

Two interacting galaxies known as Arp 142 in a horizontal image taken in mid-infrared light. At left is NGC 2937, an elliptical galaxy that looks like a tiny teal oval and is nicknamed the Egg. At right is NGC 2936, a distorted spiral galaxy nicknamed the Penguin, which is significantly larger. A beak-like region points toward the Egg, but lies far above it. Where the eye would be is an opaque, almost washed-out pink spiral. This galaxy’s distorted pink, purple, and blue arms create the bird’s beak, back, and tail. The tail, which is closer to the Egg, is wide and layered, like a beta fish’s tail. The Penguin and the Egg appear very separate. The galaxy at top right, PGC 1237172, is barely visible. A brighter slightly larger blue foreground star that is overtop this galaxy has tiny diffraction spikes. Throughout the image are tiny galaxies in bright reds, greens, and blues. The background of space is black.
NASA’s James Webb Space Telescope’s mid-infrared view of interacting galaxies Arp 142 seems to sing in primary colors. The Egg shows up as a tiny, teal-colored oval, because it is made up of old stars and has lost or used up most of its gas and dust. At right, the Penguin’s star-forming regions are represented in pink and purple, and contain smoke-like material known as polycyclic aromatic hydrocarbons.

Also take a moment to scan the background. Webb’s image is overflowing with distant galaxies. Some take spiral and oval shapes, like those threaded throughout the Penguin’s “tail feathers,” while others scattered throughout are shapeless dots. This is a testament to the sensitivity and resolution of the telescope’s infrared instruments. (Compare Webb’s view to the 2018 observation that combines infrared light from NASA’s retired Spitzer Space Telescope and near-infrared and visible light from NASA’s Hubble Space Telescope.) Even though these observations only took a few hours, Webb revealed far more distant, redder, and dustier galaxies than previous telescopes – one more reason to expect Webb to continue to expand our understanding of everything in the universe.

Want more? Take a tour to the image, “fly through” it in a visualization, and compare Webb’s image to the Hubble Space Telescope’s.

Arp 142 lies 326 million light-years from Earth in the constellation Hydra.

Video: Tour the Arp 142 Image

Video tour transcript
Credit: NASA, ESA, CSA, STScI, Danielle Kirshenblat (STScI)

Video: Arp 142 Visualization

Credit: NASA, ESA, CSA, Ralf Crawford (STScI), Joseph DePasquale (STScI), Christian Nieves (STScI), Joseph Olmsted (STScI), Alyssa Pagan (STScI), Frank Summers (STScI), Greg Bacon (STScI)

Image C: Compare Hubble/Webb

Image Before/After

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).

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Media Contacts

Laura Betzlaura.e.betz@nasa.gov, Rob Gutrorob.gutro@nasa.gov
NASA’s Goddard Space Flight Center, Greenbelt, Md.

Claire Blomecblome@stsci.edu Christine Pulliamcpulliam@stsci.edu
Space Telescope Science Institute, Baltimore, Md.

Video: Learn more about Arp 142 and galaxy collisions
Video: Learn more about galactic collisions
Video: What happens when galaxies collide?
Interactive: Explore “Interacting Galaxies: Future of the Milky Way”
Video: Galaxy Collisions: Simulations vs. Observations
Article: More about Galaxy Evolution

More Webb News

More Webb Images

Webb Mission Page

What is a galaxy?

What is the Webb Telescope?

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      Photo 4. Saswati Das takes a break from her Ph.D studies at nearby Virginia Tech (located in Blacksburg, VA) to enjoy the famous fall colors in the mountains of West Virginia. Photo credit: Saswati Das The research presented that week spanned a variety of topics. OCO-2 was being used to develop early drought forecasts. Because of its ability to detect the SIF “glow” that results from plant photosynthesis, OCO-2 can hint at flash droughts as early as three months before environmental decay unfold. By pairing OCO-2 data from other satellites, such as soil moisture data from NASA’s Soil Moisture Active Passive (SMAP) mission, scientists have opened a new window into drought forecasts and how water supply affects plant growth.
      Surprises about our planet have also emerged. The tropical rainforests, long nicknamed the “lungs” of our planet, don’t always inhale and store carbon. At times, this region can exhale CO2, such as during the 2015–2016 El Niño. That period saw large tropical forests temporarily transform into net carbon sources – see Figure 5. The driver for this shift varied by region. The Amazon rainforest was driven by drought. Central Africa was driven by unusually high temperatures. Indonesia was driven by widespread fires.
      Figure 5. The 2015–2016 El Niño increased the net carbon dioxide released by Earth’s tropical regions into the atmosphere. Figure credit: NASA-JPL/Caltech Data from OCO-2 and OCO-3 have also been used to study emissions from both cities and large power plants. This approach offers a new way to track changing emissions over time – without needing to continuously measure them on the ground. In addition, scientists are combining the satellite data with wind models and urban maps to trace CO2 to its sources (e.g., factories, ships, and roadways), helping to disentangle emissions from overlapping city sectors. These methods have been used to isolate industrial emissions in places, such as Europe, China, as well as over cities, such as Los Angeles, Paris, and Seoul. It has also revealed pandemic-era drops in traffic-related CO2 and increases in CO2 tied to shipping backlogs at the port. Two representatives from the World Bank shared how they used data from OCO-2 to demonstrate that building subway systems in cities can lower emissions. The goal is to eventually use these tools to evaluate local strategies (e.g., bike lanes and public transit) to reduce local carbon footprints.
      When massive wildfires blazed through Australian forests and bushland in 2019, researchers used OCO-2 data to study the unfolding crisis. OCO-2 captured the increase in atmospheric CO2, and scientists used this data to refine estimates of how these events contribute to the global carbon budget.
      As her mind wandered from the rich research she’d been immersed in for the past hour, Saswati spied Otto Lamminpää across the aisle in the wood-paneled auditorium. She thought back to the forests she loved on the East Coast, and the forests in Finland where Otto had grown up. OCO-2 was telling a story about the role that forests play in absorbing carbon and how this has changed over time.
      2025 and Beyond
      The Tapestry Continues to Expand…
      In many ways, OCO-2 has had a long and unexpected journey. So has Hannah Murphy, another DEVELOP intern who will be starting a Master’s degree at Hunter College in New York in Fall 2025. She’s studied art and worked as a set designer in Los Angeles. She never pictured herself working with satellite data, but then she saw how visual it could be. The glowing, evocative images of Earth from space spoke to her artistic heart.
      Now, Hannah works on SIF data as a 2025 NASA DEVELOP intern with the OCO-2 team, developing tools for wildfire risks. This project in particular hits close to home for Hannah, because she lived through the wildfires that tore through Los Angeles in January 2025. Although she remained safe, she knew several people who lost their homes, and the air was unsafe to breathe for weeks.
      Just a few short months later, Hannah began studying the data from OCO-2. She is now part of the new generation of researchers that will take the mission’s remote sensing data and pave the way for implementing the findings to benefit society. Hannah understands, on a personal level, how closely our lives are linked to Earth systems that satellites, such as OCO-2 and OCO-3, study from space.
      OCO-2 (and OCO-3) are built to study CO2 and plant health, but its impact goes deeper to the connections that tie our atmosphere, ecosystems, and lives together. That work continues to the new generation of scientists – one breath at a time.
      Mejs Hasan
      NASA/Jet Propulsion Laboratory
      mejs.hasan@jpl.nasa.gov
      Alan Ward
      NASA’s Goddard Space Flight Center/Global Science & Technology Inc.
      alan.b.ward@nasa.gov
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      Last Updated Aug 12, 2025 Related Terms
      Earth Science View the full article
    • By NASA
      Credit: NASA NASA has selected KBR Wyle Services, LLC of Fulton, Maryland, to provide services to the Human Health and Performance Directorate at the agency’s Johnson Space Center in Houston, which focuses on astronaut health, occupational health, and research that could help mitigate health risks for future human spaceflight missions.
      The Human Health and Performance Contract 2 is a follow-on single-award indefinite-delivery/indefinite-quantity contract that begins its five-year period of performance on Nov. 1, with two possible option periods that could extend it through 2035. The total estimated value of the base period plus the optional periods is $3.6 billion. Leidos, Inc. of Reston, Virginia, is a subcontractor.
      The contract will acquire support services for several programs, primarily at NASA Johnson. This includes the Human Research Program, International Space Station Program, Commercial Crew Program, Artemis campaign, and more. Services include ensuring crew health, safety, and performance; providing occupational health services; and conducting research into mitigating risks to the health, safety, and performance of future spaceflight crews.
      The Human Health and Performance Directorate leads the global spaceflight community in protecting astronaut health and enabling human mission performance. Its vision focuses on humans living, working, and thriving in space, on the Moon and on to Mars, and its mission is to lead the global spaceflight community in protecting astronaut health and enabling human mission performance.
      For more information about NASA and agency programs, visit:
      https://www.nasa.gov
      –end–
      Tiernan Doyle
      Headquarters, Washington
      202-358-1600
      tiernan.doyle@nasa.gov
      Victoria Segovia
      Johnson Space Center, Houston
      281-483-5111
      victoria.segovia@nasa.gov
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      Last Updated Aug 11, 2025 LocationNASA Headquarters Related Terms
      Johnson Space Center Human Health and Performance NASA Centers & Facilities View the full article
    • By NASA
      NASA Second Lady Usha Vance and NASA Astronaut Suni Williams listen to the audience in this image from Aug. 4, 2025. Ms. Vance joined Williams at NASA’s Johnson Space Center in Houston for a summer reading challenge event, through which the Second Lady encourages youth to seek adventure, imagination, and discovery between the pages of a book.
      Image credit: NASA
      View the full article
    • By NASA
      The Crew Health and Performance Exploration Analog (CHAPEA) team hosts a media day at NASA’s Johnson Space Center in Houston in 2023.Credit: NASA As NASA prepares for its second year-long Mars simulated mission, media are invited to visit the ground-based habitat where the mission will take place, on Friday, Aug. 22, at the agency’s Johnson Space Center in Houston.
      Scheduled to begin in October, four volunteer crew members will enter the agency’s Crew Health and Performance Exploration Analog (CHAPEA) 3D-printed habitat to live and work for a year to inform NASA’s preparations for human Mars missions.
      The in-person media event includes an opportunity to speak with subject matter experts, and capture b-roll and photos inside the habitat. Crew members will not be available for interviews as they will arrive at NASA Johnson at a later date.
      International media wishing to attend must request accreditation no later than 6 p.m. EDT (5 p.m. CDT), on Monday, Aug. 11. United States-based media have a deadline of 6 p.m. EDT (5 p.m. CDT), on Wednesday, Aug. 20, to register.  
      To request accreditation, media must contact the NASA Johnson newsroom at: 281-483-5111 or jsccommu@mail.nasa.gov. Space is limited. A copy of NASA’s media accreditation policy is available online.
      Once the crew members kick off their mission, they will carry out various activities, including simulated Mars walks, robotic operations, habitat maintenance, medical technology tests, exercise, and crop growth. The crew also will face environmental stresses such as resource limitations, isolation, communication delays, and equipment failure, and work through these scenarios with the resources available inside the habitat.
      To learn more about CHAPEA, visit:
      https://www.nasa.gov/humans-in-space/chapea
      -end-
      Lauren Low
      Headquarters, Washington
      202-358-1600
      lauren.e.low@nasa.gov
      Kelsey Spivey / Mohi Kumar
      Johnson Space Center, Houston
      281-483-5111
      kelsey.m.spivey@nasa.gov / mohi.kumar@nasa.gov
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      Last Updated Aug 04, 2025 LocationNASA Headquarters Related Terms
      Crew Health and Performance Exploration Analog (CHAPEA) Humans in Space Johnson Space Center View the full article
    • By NASA
      Second Lady Visits NASA for Summer Reading Challenge
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