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NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets

NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets
NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets

4 Min Read

NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets

Near the center is an object that resembles an edge-on view of a hamburger. There is a diagonal dark strip (the meat patty) of dust, running from 1 o'clock to 7 o'clock, that obscures a central star. Curving away from either side of the dark strip are glowing white clouds (the buns) where dust is reflecting starlight. Bright blue finger-like wisps of material extend far above and below the dark center plane. A few dozen stars, some with four diffraction spikes, are scattered on the black background of space.

Astronomers using NASA’s Hubble Space Telescope have imaged the largest protoplanetary disk ever observed circling a young star. For the first time in visible light, Hubble has revealed the disk is unexpectedly chaotic and turbulent, with wisps of material stretching much farther above and below the disk than astronomers have seen in any similar system. Strangely, more extended filaments are only visible on one side of the disk. The findings, which published Tuesday in The Astrophysical Journal, mark a new milestone for Hubble and shed light on how planets may form in extreme environments, as NASA’s missions lead humanity’s exploration of the universe and our place in it.

Located roughly 1,000 light-years from Earth, IRAS 23077+6707, nicknamed “Dracula’s Chivito,” spans nearly 400 billion miles — 40 times the diameter of our solar system to the outer edge of the Kuiper Belt of cometary bodies. The disk obscures the young star within it, which scientists believe may be either a hot, massive star, or a pair of stars. And the enormous disk is not only the largest known planet-forming disk; it’s also shaping up to be one of the most unusual.

“The level of detail we’re seeing is rare in protoplanetary disk imaging, and these new Hubble images show that planet nurseries can be much more active and chaotic than we expected,” said lead author Kristina Monsch of the Center for Astrophysics | Harvard & Smithsonian (CfA). “We’re seeing this disk nearly edge-on and its wispy upper layers and asymmetric features are especially striking. Both Hubble and NASA’s James Webb Space Telescope have glimpsed similar structures in other disks, but IRAS 23077+6707 provides us with an exceptional perspective — allowing us to trace its substructures in visible light at an unprecedented level of detail. This makes the system a unique, new laboratory for studying planet formation and the environments where it happens.”

The nickname “Dracula’s Chivito” playfully reflects the heritage of its researchers—one from Transylvania and another from Uruguay, where the national dish is a sandwich called a chivito. The edge-on disk resembles a hamburger, with a dark central lane flanked by glowing top and bottom layers of dust and gas.

Near the center is an object that resembles an edge-on view of a hamburger. There is a diagonal dark strip (the meat patty) of dust, running from 1 o'clock to 7 o'clock, that obscures a central star. Curving away from either side of the dark strip are glowing white clouds (the buns) where dust is reflecting starlight. Bright blue finger-like wisps of material extend far above and below the dark center plane. A few dozen stars, some with four diffraction spikes, are scattered on the black background of space.
This Hubble Space Telescope image shows the largest planet-forming disk ever observed around a young star. It spans nearly 400 billion miles — 40 times the diameter of our solar system.
Image: NASA, ESA, STScI, Kristina Monsch (CfA); Image Processing: Joseph DePasquale (STScI)

Puzzling asymmetry

The impressive height of these features wasn’t the only thing that captured the attention of scientists. The new images revealed that vertically imposing filament-like features appear on just one side of the disk, while the other side appears to have a sharp edge and no visible filaments. This peculiar, lopsided structure suggests that dynamic processes, like the recent infall of dust and gas, or interactions with its surroundings, are shaping the disk.

“We were stunned to see how asymmetric this disk is,” said co-investigator Joshua Bennett Lovell, also an astronomer at the CfA. “Hubble has given us a front row seat to the chaotic processes that are shaping disks as they build new planets — processes that we don’t yet fully understand but can now study in a whole new way.”

All planetary systems form from disks of gas and dust encircling young stars. Over time, the gas accretes onto the star, and planets emerge from the remaining material. IRAS 23077+6707 may represent a scaled-up version of our early solar system, with a disk mass estimated at 10 to 30 times that of Jupiter — ample material for forming multiple gas giants. This, plus the new findings, makes it an exceptional case for studying the birth of planetary systems.

“In theory, IRAS 23077+6707 could host a vast planetary system,” said Monsch. “While planet formation may differ in such massive environments, the underlying processes are likely similar. Right now, we have more questions than answers, but these new images are a starting point for understanding how planets form over time and in different environments.”

Credit: NASA’s Goddard Space Flight Center; Lead Producer: Paul Morris

The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.

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Related Images & Videos

Near the center is an object that resembles an edge-on view of a hamburger. There is a diagonal dark strip (the meat patty) of dust, running from 1 o'clock to 7 o'clock, that obscures a central star. Curving away from either side of the dark strip are glowing white clouds (the buns) where dust is reflecting starlight. Bright blue finger-like wisps of material extend far above and below the dark center plane. A few dozen stars, some with four diffraction spikes, are scattered on the black background of space.

Dracula’s Chivito (IRAS 23077+6707)

This Hubble Space Telescope image shows the largest planet-forming disk ever observed around a young star. It spans nearly 400 billion miles — 40 times the diameter of our solar system.

Dracula’s Chivito (IRAS 23077+6707) Compass Image

Image of Dracula’s Chivito captured by Hubble’s WFC3 instrument, with compass arrows, scale bar, and color key for reference.

Near the center is an object that resembles an edge-on view of a hamburger. There is a diagonal dark strip (the meat patty) of dust, running from 1 o'clock to 7 o'clock, that obscures a central star. Curving away from either side of the dark strip are glowing white clouds (the buns) where dust is reflecting starlight. Bright blue finger-like wisps of material extend far above and below the dark center plane. A few dozen stars, some with four diffraction spikes, are scattered on the black background of space.

Hubble Spots Giant Vampire Sandwich? Video

Dracula’s Chivito isn’t just the largest protoplanetary disk ever imaged, it’s also a window into how planets are born and how systems like our solar system may have formed.

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Last Updated

Dec 23, 2025

Editor
Andrea Gianopoulos
Location
NASA Goddard Space Flight Center
Contact

Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov

Christine Pulliam
Space Telescope Science Institute
Baltimore, Maryland

Amy Oliver
Center for Astrophysics | Harvard & Smithsonian
Cambridge, Massachusetts

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Source Link NASA’s Hubble Reveals Largest Found Chaotic Birthplace of Planets

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NASA’s SPHEREx Observatory Completes First Cosmic Map Like No Other

NASA’s SPHEREx Observatory Completes First Cosmic Map Like No Other
NASA’s SPHEREx Observatory Completes First Cosmic Map Like No Other
NASA’s SPHEREx Observatory Completes First Cosmic Map Like No Other
NASA’s SPHEREx Observatory Completes First Cosmic Map Like No Other
NASA’s SPHEREx Observatory Completes First Cosmic Map Like No Other
NASA’s SPHEREx Observatory Completes First Cosmic Map Like No Other

6 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

This panoramic view of SPHEREx’s first all-sky map shows how the sky looks to the telescope. It transitions between observations of colors emitted by hot hydrogen gas (blue) and cosmic dust (red), and those primarily emitted by stars.
Credit: NASA/JPL-Caltech

Launched in March, NASA’s SPHEREx space telescope has completed its first infrared map of the entire sky in 102 colors. While not visible to the human eye, these 102 infrared wavelengths of light are prevalent in the cosmos, and observing the entire sky this way enables scientists to answer big questions, including how a dramatic event that occurred in the first billionth of a trillionth of a trillionth of a second after the big bang influenced the 3D distribution of hundreds of millions of galaxies in our universe. In addition, scientists will use the data to study how galaxies have changed over the universe’s nearly 14 billion-year history and learn about the distribution of key ingredients for life in our own galaxy.  

“It’s incredible how much information SPHEREx has collected in just six months — information that will be especially valuable when used alongside our other missions’ data to better understand our universe,” said Shawn Domagal-Goldman, director of the Astrophysics Division at NASA Headquarters in Washington. “We essentially have 102 new maps of the entire sky, each one in a different wavelength and containing unique information about the objects it sees. I think every astronomer is going to find something of value here, as NASA’s missions enable the world to answer fundamental questions about how the universe got its start, and how it changed to eventually create a home for us in it.” 

Circling Earth about 14½ times a day, SPHEREx (which stands for Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer) travels from north to south, passing over the poles. Each day it takes about 3,600 images along one circular strip of the sky, and as the days pass and the planet moves around the Sun, SPHEREx’s field of view shifts as well. After six months, the observatory has looked out into space in every direction, capturing the entire sky in 360 degrees. 

Managed by NASA’s Jet Propulsion Laboratory in Southern California, the mission began mapping the sky in May and completed its first all-sky mosaic in December. It will complete three additional all-sky scans during its two-year primary mission, and merging those maps together will increase the sensitivity of the measurements. The entire dataset is freely available to scientists and the public.  

“SPHEREx is a mid-sized astrophysics mission delivering big science,” said JPL Director Dave Gallagher. “It’s a phenomenal example of how we turn bold ideas into reality, and in doing so, unlock enormous potential for discovery.”  

Superpowered telescope 

Each of the 102 colors detected by SPHEREx represents a wavelength of infrared light, and each wavelength provides unique information about the galaxies, stars, planet-forming regions, and other cosmic features therein. For example, dense clouds of dust in our galaxy where stars and planets form radiate brightly in certain wavelengths but emit no light (and are therefore totally invisible) in others. The process of separating the light from a source into its component wavelengths is called spectroscopy.  

And while a handful of previous missions has also mapped the entire sky, such as NASA’s Wide-field Infrared Survey Explorer, none have done so in nearly as many colors as SPHEREx. By contrast, NASA’s James Webb Space Telescope can do spectroscopy with significantly more wavelengths of light than SPHEREx, but with a field of view thousands of times smaller. The combination of colors and such a wide field of view is why SPHEREx is so powerful. 

“The superpower of SPHEREx is that it captures the whole sky in 102 colors about every six months. That’s an amazing amount of information to gather in a short amount of time,” said Beth Fabinsky, the SPHEREx project manager at JPL. “I think this makes us the mantis shrimp of telescopes, because we have an amazing multicolor visual detection system and we can also see a very wide swath of our surroundings.” 

To accomplish this feat, SPHEREx uses six detectors, each paired with a specially designed filter that contains a gradient of 17 colors. That means every image taken with those six detectors contains 102 colors (six times 17). It also means that every all-sky map that SPHEREx produces is really 102 maps, each in a different color.  

The observatory will use those colors to measure the distance to hundreds of millions of galaxies. Though the positions of most of those galaxies have already been mapped in two dimensions by other observatories, SPHEREx’s map will be in 3D, enabling scientists to measure subtle variations in the way galaxies are clustered and distributed across the universe.  

Each frame of this movie shows the entire sky in a different infrared wavelength, indicated by the color bar in the top right corner. Taken by NASA’s SPHEREx observatory, the maps illustrate how viewing the universe in different wavelengths of light can reveal unique cosmic features.
Credit: NASA/JPL-Caltech

Those measurements will offer insights into an event that took place in the first billionth of a trillionth of a trillionth of a second after the big bang. In this moment, called inflation, the universe expanded by a trillion-trillionfold. Nothing like it has occurred in the universe since, and scientists want to understand it better. The SPHEREx mission’s approach is one way to help in that effort. 

More about SPHEREx 

The SPHEREx mission is managed by JPL for NASA’s Astrophysics Division within the Science Mission Directorate in Washington. The telescope and the spacecraft bus were built by BAE Systems. The science analysis of the SPHEREx data is being conducted by a team of scientists at 10 institutions across the U.S., and in South Korea and Taiwan. Data is processed and archived at IPAC at Caltech in Pasadena, which manages JPL for NASA. The mission’s principal investigator is based at Caltech with a joint JPL appointment. The SPHEREx dataset is publicly available. 

For more information about the SPHEREx mission visit: 

https://science.nasa.gov/mission/spherex/

News Media Contacts

Calla Cofield 
Jet Propulsion Laboratory, Pasadena, Calif. 
626-808-2469 
calla.e.cofield@jpl.nasa.gov 

2025-144

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Last Updated

Dec 18, 2025

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NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time

NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time
NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time

5 Min Read

NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time

A grainy orange oval ring tilts slightly from upper right to lower left.

Like a game of cosmic bumper cars, scientists think the early days of our solar system were a time of violent turmoil, with planetesimals, asteroids, and comets smashing together and pelting the Earth, Moon, and the other inner planets with debris. Now, in a historical milestone, NASA’s Hubble Space Telescope has directly imaged similar catastrophic collisions in a nearby planetary system around another star, Fomalhaut.

“This is certainly the first time I’ve ever seen a point of light appear out of nowhere in an exoplanetary system,” said principal investigator Paul Kalas of the University of California, Berkeley. “It’s absent in all of our previous Hubble images, which means that we just witnessed a violent collision between two massive objects and a huge debris cloud unlike anything in our own solar system today. Amazing!”

Just 25 light-years from Earth, Fomalhaut is one of the brightest stars in the night sky. Located in the constellation Piscis Austrinus, also known as the Southern Fish, it is more massive and brighter than the Sun and is encircled by several belts of dusty debris.

Image labeled Fomalhaut system, Hubble Space Telescope. A grainy orange oval ring tilts slightly from upper right to lower left. At two o'clock, a white box outlines the ring's edge and white lines extend to a larger pullout box at lower right. Two spots inside the larger box are marked with dashed white circles and labeled cs1 2012 and cs2 2023. Inside the ring is a black circle with a white star symbol in the middle.
This composite Hubble Space Telescope image shows the debris ring and dust clouds cs1 and cs2 around the star Fomalhaut. Fomalhaut itself is masked out to allow the fainter features to be seen. Its location is marked by the white star.
Image: NASA, ESA, Paul Kalas (UC Berkeley); Image Processing: Joseph DePasquale (STScI)

In 2008, scientists used Hubble to discover a candidate planet around Fomalhaut, making it the first stellar system with a possible planet found using visible light. That object, called Fomalhaut b, now appears to be a dust cloud masquerading as a planet—the result of colliding planetesimals. While searching for Fomalhaut b in recent Hubble observations, scientists were surprised to find a second point of light at a similar location around the star. They call this object “circumstellar source 2” or “cs2” while the first object is now known as “cs1.”

Tackling Mysteries of Colliding Planetesimals

Why astronomers are seeing both of these debris clouds so physically close to each other is a mystery. If the collisions between asteroids and planetesimals were random, cs1 and cs2 should appear by chance at unrelated locations. Yet, they are positioned intriguingly near each other along the inner portion of Fomalhaut’s outer debris disk.

Another mystery is why scientists have witnessed these two events within such a short timeframe. “Previous theory suggested that there should be one collision every 100,000 years, or longer. Here, in 20 years, we’ve seen two,” explained Kalas. “If you had a movie of the last 3,000 years, and it was sped up so that every year was a fraction of a second, imagine how many flashes you’d see over that time. Fomalhaut’s planetary system would be sparkling with these collisions.”

Collisions are fundamental to the evolution of planetary systems, but they are rare and difficult to study.

Illustration is labeled Artist’s Concept in the bottom left corner. This four-panel image shows the sequence of events leading up to, during, and following the collision of two objects in orbit around a star. Please refer to the Extended Description for more details.
This artist’s concept shows the sequence of events leading up to the creation of dust cloud cs2 around the star Fomalhaut. In Panel 1, the star Fomalhaut appears in the top left corner. Two white dots, located in the bottom right corner, represent the two massive objects in orbit around Fomalhaut. In Panel 2, the objects approach each other. Panel 3 shows the violent collision of these two objects. In Panel 4, the resulting dust cloud cs2 becomes visible and starlight pushes the dust grains away from the star.
Artwork: NASA, ESA, STScI, Ralf Crawford (STScI)

“The exciting aspect of this observation is that it allows researchers to estimate both the size of the colliding bodies and how many of them there are in the disk, information which is almost impossible to get by any other means,” said co-author Mark Wyatt at the University of Cambridge in England. “Our estimates put the planetesimals that were destroyed to create cs1 and cs2 at just 37 miles or 60 kilometers across, and we infer that there are 300 million such objects orbiting in the Fomalhaut system.”

“The system is a natural laboratory to probe how planetesimals behave when undergoing collisions, which in turn tells us about what they are made of and how they formed,” explained Wyatt.

Cautionary Tale

The transient nature of Fomalhaut cs1 and cs2 poses challenges for future space missions aiming to directly image exoplanets. Such telescopes may mistake dust clouds like cs1 and cs2 for actual planets.

“Fomalhaut cs2 looks exactly like an extrasolar planet reflecting starlight,” said Kalas. “What we learned from studying cs1 is that a large dust cloud can masquerade as a planet for many years. This is a cautionary note for future missions that aim to detect extrasolar planets in reflected light.”

Looking to Future

Kalas and his team have been granted Hubble time to monitor cs2 over the next three years. They want to see how it evolves—does it fade, or does it get brighter? Being closer to the dust belt than cs1, the expanding cs2 cloud is more likely to start encountering other material in the belt. This could lead to a sudden avalanche of more dust in the system, which could cause the whole surrounding area to get brighter.

Credit: NASA’s Goddard Space Flight Center; Lead Producer: Paul Morris

“We will be tracing cs2 for any changes in its shape, brightness, and orbit over time,” said Kalas, “It’s possible that cs2 will start becoming more oval or cometary in shape as the dust grains are pushed outward by the pressure of starlight.”

The team also will use the NIRCam (Near-Infrared Camera) instrument on NASA’s James Webb Space Telescope to observe cs2. Webb’s NIRCam has the ability to provide color information that can reveal the size of the cloud’s dust grains and their composition. It can even determine if the cloud contains water ice. 

Hubble and Webb are the only observatories capable of this kind of imaging. While Hubble primarily sees in visible wavelengths, Webb could view cs2 in the infrared. These different, complementary wavelengths are needed to provide a broad multi-spectral investigation and a more complete picture of the mysterious Fomalhaut system and its rapid evolution.

This research appears in the December 18 issue of Science.

The Hubble Space Telescope has been operating for over three decades and continues to make ground-breaking discoveries that shape our fundamental understanding of the universe. Hubble is a project of international cooperation between NASA and ESA (European Space Agency). NASA’s Goddard Space Flight Center in Greenbelt, Maryland, manages the telescope and mission operations. Lockheed Martin Space, based in Denver, also supports mission operations at Goddard. The Space Telescope Science Institute in Baltimore, which is operated by the Association of Universities for Research in Astronomy, conducts Hubble science operations for NASA.

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Image labeled Fomalhaut system, Hubble Space Telescope. A grainy orange oval ring tilts slightly from upper right to lower left. At two o'clock, a white box outlines the ring's edge and white lines extend to a larger pullout box at lower right. Two spots inside the larger box are marked with dashed white circles and labeled cs1 2012 and cs2 2023. Inside the ring is a black circle with a white star symbol in the middle.

Fomalhaut cs2

This composite Hubble Space Telescope image shows the debris ring and dust clouds cs1 and cs2 around the star Fomalhaut. Fomalhaut itself is masked out to allow the fainter features to be seen. Its location is marked by the white star.

Illustration is labeled Artistu2019s Concept in the bottom, left corner. Slightly off-center against a black background, an explosive and fiery-looking orange object appears. Orange streamers, filaments, and particles radiate from the objectu2019s center. Within it, but slightly off-center to the right, is a mottled, yellow, amorphous blob. This blob is outlined on three sides in white, and on the fourth, right side in dark orange and red. White particles emanate from this blob, particularly on the right side.

Fomalhaut cs2 Illustration

This artist’s concept shows the sequence of events leading up to the creation of dust cloud cs2 around the star Fomalhaut.

At the top left corner, a fuzzy white star appears. Traversing the top of the image and cutting across the top of the star is a ghostly white streak. At the bottom right corner is an explosive and fiery-looking orange object. Orange streamers, filaments, and particles radiate from the objectu2019s center. Within it, but slightly off-center to the right, is a mottled, yellow, amorphous blob. This blob is outlined on three sides in white, and on the fourth, right side in dark orange and red. White particles emanate from this blob, particularly on the right side.

Fomalhaut cs2 Video

Hubble captured the violent collision of two massive objects around the star Fomalhaut. This extraordinary event is unlike anything in our own present-day solar system. The video shows the sequence of events leading up to the creation of dust cloud cs2 around the star Fomalhaut. …

A grainy orange oval ring tilts slightly from upper right to lower left.

Hubble Captures Destruction of Worlds Video

NASA’s Hubble Space Telescope captured a rare and violent event unfolding around the nearby star Fomalhaut. This discovery sheds light on the chaotic processes that may have shaped our own solar system billions of years ago. With support from both Hubble and the James Webb Space Telescope, astronomers are now closely monitoring the aftermath.

Model of Fomalhaut b Dust Cloud

From 2020:
Exoplanet Apparently Disappears in Latest Hubble Observations

What astronomers thought was a planet beyond our solar system has now seemingly vanished from sight. 

Rogue Planetary Orbit for Fomalhaut b

From 2013:
Hubble Reveals Rogue Planetary Orbit for Fomalhaut b

Newly released Hubble Space Telescope images of a vast debris disk encircling the nearby star Fomalhaut, and of a mysterious planet circling it, may provide forensic evidence of a titanic planetary disruption in the system.

HST Image of Fomalhaut and Fomalhaut b

From 2008:
Hubble Directly Observes Planet Orbiting Fomalhaut

NASA’s Hubble Space Telescope has taken the first visible-light snapshot of a planet circling another star.

Fomalhaut Debris Ring (Annotated)

From 2005:
Elusive Planet Reshapes a Ring Around Neighboring Star

NASA Hubble Space Telescope’s most detailed visible-light image ever taken of a narrow, dusty ring around the nearby star Fomalhaut (HD 216956), offers the strongest evidence yet that an unruly and unseen planet may be gravitationally tugging on the ring.

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Details

Last Updated

Dec 19, 2025

Editor
Andrea Gianopoulos
Location
NASA Goddard Space Flight Center
Contact

Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov

Ann Jenkins, Christine Pulliam
Space Telescope Science Institute
Baltimore, Maryland

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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 Science Highlights


Hubble Images


Hubble News

Source Link NASA’s Hubble Sees Asteroids Colliding at Nearby Star for First Time

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Hubble Glimpses Galactic Gas Making a Getaway

Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway
Hubble Glimpses Galactic Gas Making a Getaway

2 min read

Hubble Glimpses Galactic Gas Making a Getaway

A nearly edge-on spiral galaxy. Its disk holds pink light from star-forming nebulae and blue light from clusters of hot stars. Thick dark clouds of dust block the strong white light from galaxy’s center. A faint, glowing halo of gas surrounds the disk, fading into the black background of space. A bluish plume of gas also extends from the galaxy’s core extending toward the lower-right corner of the image.
This NASA/ESA Hubble Space Telescope image features the galaxy NGC 4388, a member of the Virgo galaxy cluster.
ESA/Hubble & NASA, S. Veilleux, J. Wang, J. Greene

A sideways spiral galaxy shines in this NASA/ESA Hubble Space Telescope image. Located about 60 million light-years away in the constellation Virgo (the Maiden), NGC 4388 is a resident of the Virgo galaxy cluster. This enormous cluster of galaxies contains more than a thousand members and is the nearest large galaxy cluster to the Milky Way.

NGC 4388 appears to tilt at an extreme angle relative to our point of view, giving us a nearly edge-on prospect of the galaxy. This perspective reveals a curious feature that wasn’t visible in a previous Hubble image of this galaxy released in 2016: a plume of gas from the galaxy’s nucleus, here seen billowing out from the galaxy’s disk toward the lower-right corner of the image. But where did this outflow come from, and why does it glow?

The answer likely lies in the vast stretches of space that separate the galaxies of the Virgo cluster. Though the space between galaxies appears empty, this space is occupied by hot wisps of gas called the intracluster medium. As NGC 4388 moves within the Virgo cluster, it plunges through the intracluster medium. Pressure from hot intracluster gas whisks away gas from within NGC 4388’s disk, causing it to trail behind as NGC 4388 moves.

The source of the ionizing energy that causes this gas cloud to glow is more uncertain. Researchers suspect that some of the energy comes from the center of the galaxy, where a supermassive black hole spins gas around it into a superheated disk. The blazing radiation from this disk might ionize the gas closest to the galaxy, while shock waves might be responsible for ionizing filaments of gas farther out.

This image incorporates new data, including several additional wavelengths of light, that bring the ionized gas cloud into view. The image holds data from several observing programs that aim to illuminate galaxies with active black holes at their centers.

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Claire Andreoli (claire.andreoli@nasa.gov)
NASA’s Goddard Space Flight Center, Greenbelt, MD

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Dec 18, 2025

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NASA IXPE’s Longest Observation Solves Black Hole Jets Mystery

NASA IXPE’s Longest Observation Solves Black Hole Jets Mystery
NASA IXPE’s Longest Observation Solves Black Hole Jets Mystery
NASA IXPE’s Longest Observation Solves Black Hole Jets Mystery

4 min read

Preparations for Next Moonwalk Simulations Underway (and Underwater)

The Perseus Cluster. Left: Imaging X-ray Polarimetry Explorer (IXPE); Right: Chandra X-ray Observatory.
Two composite images show side-by-side observations of the Perseus Cluster from NASA’s IXPE (Imaging X-Ray Polarimetry Explorer) and Chandra X-ray Observatory. Scientists used data from both observatories, along with data from Nuclear Spectroscopic Telescope Array (NuSTAR), and Neil Gehrels Swift Observatory, to confirm measurements of the galaxy cluster.
X-ray: (Chandra) NASA/CXC/SAO, (IXPE) NASA/MSFC; Image Processing: NASA/CXC/SAO/N. Wolk and K. Arcand

Written by Michael Allen

An international team of astronomers using NASA’s IXPE (Imaging X-ray Polarimetry Explorer) has identified the origin of X-rays in a supermassive black hole’s jet, answering a question that has been unresolved since the earliest days of X-ray astronomy. Their findings are described in a paper published in The Astrophysical Journal Letters, by the American Astronomical Society, Nov. 11.

The IXPE mission observed the Perseus Cluster, the brightest galaxy cluster i observable in X-rays, for more than 600 hours over a 60-day period between January and March. Not only is this IXPE’s longest observation of a single target to date, it also marks IXPE’s first time observing a galaxy cluster.

Specifically, the team of scientists studied the polarization properties of 3C 84, the massive active galaxy located at the very center of the Perseus Cluster. This active galaxy is a well-known X-ray source and a common target for X-ray astronomers because of its proximity and brightness.

Because the Perseus Cluster is so massive, it hosts an enormous reservoir of X-ray emitting gas as hot as the core of the Sun. The use of multiple X-ray telescopes, particularly the high-resolution imaging power of NASA’s Chandra X-ray Observatory was essential to disentangle the signals in the IXPE data. Scientists combined these X-ray measurements with data from the agency’s Nuclear Spectroscopic Telescope Array (NuSTAR) mission and Neil Gehrels Swift Observatory.

Fast facts

  • Polarization measurements from IXPE carry information about the orientation and alignment of emitted X-ray light waves. The more X-ray waves traveling in sync, the higher the degree of polarization.
  • X-rays from an active galaxy like 3C 84 are thought to originate from a process known as inverse Compton scattering, where light bounces off particles and gains energy. The polarization measurements from IXPE allow us to identify the presence of either inverse Compton scattering or other scenarios.
  • “Seed photons” is the term for the lower-energy radiation undergoing the energizing process of inverse Compton scattering.
  • You may remember the Perseus Cluster from this sonification replicating what a Black Hole sounds like from May 2022.

“While measuring the polarization of 3C 84 was one of the key science goals, we are still searching for additional polarization signals in this galaxy cluster that could be signatures of more exotic physics,” said Steven Ehlert, project scientist for IXPE and astronomer at NASA’s Marshall Space Flight Center in Huntsville.

Chandra & IXPE composite image of the Perseus Cluster.
Chandra & IXPE composite image of the Perseus Cluster.
X-ray: (Chandra) NASA/CXC/SAO, (IXPE) NASA/MSFC; Image Processing: NASA/CXC/SAO/N. Wolk and K. Arcand

“We’ve already determined that for sources like 3C 84, the X-rays originated from inverse Compton scattering,” said Ioannis Liodakis, a researcher at the Institute of Astrophysics – FORTH in Heraklion, Greece, and lead author on the paper. “With IXPE observations of 3C 84 we had a unique chance to determine the properties of the seed photons.”

The first possible origin scenario for the seed photons is known as synchrotron self-Compton, where lower-energy radiation originates from the same jet that produces the highly energetic particles.

In the alternative scenario known as external Compton, seed photons originate from background radiation sources unrelated to the jet.

“The synchrotron self-Compton and external Compton scenarios have very different predictions for their X-ray polarization,” said Frederic Marin, an astrophysicist at the Strasbourg Astronomical Observatory in France and co-author of the study. “Any detection of X-ray polarization from 3C 84 almost decisively rules out the possibility of external Compton as the emission mechanism.”

Throughout the 60-day observation campaign, optical and radio telescopes around the world turned their attention to 3C 84 to further test between the two scenarios.

NASA’s IXPE measured a net polarization of 4% in the X-rays spectrum, with comparable values measured in the optical and radio data. These results strongly favor the synchrotron self-Compton model for the seed photons, where they come from the same jet as the higher-energy particles.

“Separating these two components was essential to this measurement and could not be done by any single X-ray telescope, but by combining the IXPE polarization data with Chandra, NuSTAR, and Swift, we were able to confirm this polarization measurement was associated specifically with 3C 84,” said Sudip Chakraborty, a researcher at the Science and Technology Institute of the Universities Space Research Association in Huntsville, Alabama, and co-author on the paper.

Scientists will continue to analyze IXPE’s data from different locations in the Perseus Cluster for different signals.

More about IXPE

NASA’s IXPE, which continues to provide unprecedented data enabling groundbreaking discoveries about celestial objects across the universe, is a joint NASA and Italian Space Agency mission with partners and science collaborators in 12 countries. The IXPE mission is led by NASA’s Marshall Space Flight Center in Huntsville, Alabama. BAE Systems, Inc., headquartered in Falls Church, Virginia, manages spacecraft operations together with the University of Colorado’s Laboratory for Atmospheric and Space Physics in Boulder.

Learn more about IXPE’s ongoing mission here:

https://www.nasa.gov/ixpe

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Dec 16, 2025

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NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation

NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation
NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation

 

6 min read

NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation

6 Min Read

NASA’s Webb Observes Exoplanet Whose Composition Defies Explanation

llustration labeled “artist’s concept” at right bottom corner. At left bottom corner, a partially illuminated, lemon-shaped exoplanet appears against a black background. This planet is most brightly illuminated at its elongated tip on its right side. On the left side, which is wider, the planet trails off into the darkness of the background. The planet is colored in varying, mottled shades of red, light pink, and fuchsia. Most of the pink occurs closest to the tip, while most of the fuchsia is at the top and bottom edges. At right top corner, a white beam emanates diagonally, oriented from 10 o’clock to 4 o’clock, from either side of a small, glowing, white star.

This artist’s concept shows what the exoplanet called PSR J2322-2650b (left) may look like as it orbits a rapidly spinning neutron star called a pulsar (right).

Credits:
Illustration: NASA, ESA, CSA, Ralf Crawford (STScI)

Scientists using NASA’s James Webb Space Telescope have observed a rare type of exoplanet, or planet outside our solar system, whose atmospheric composition challenges our understanding of how it formed. 

Officially named PSR J2322-2650b, this Jupiter-mass object appears to have an exotic helium-and-carbon-dominated atmosphere unlike any ever seen before. Soot clouds likely float through the air, and deep within the planet, these carbon clouds can condense and form diamonds. How the planet came to be is a mystery. The paper appears Tuesday in The Astrophysical Journal Letters. 

“This was an absolute surprise,” said study co-author Peter Gao of the Carnegie Earth and Planets Laboratory in Washington. “I remember after we got the data down, our collective reaction was ‘What the heck is this?’ It’s extremely different from what we expected.”

Image A: Exoplanet PSR J2322-2650b and Pulsar (Artist’s Concept)

llustration labeled u201cartistu2019s conceptu201d at right bottom corner. At left bottom corner, a partially illuminated, lemon-shaped exoplanet appears against a black background. This planet is most brightly illuminated at its elongated tip on its right side. On the left side, which is wider, the planet trails off into the darkness of the background. The planet is colored in varying, mottled shades of red, light pink, and fuchsia. Most of the pink occurs closest to the tip, while most of the fuchsia is at the top and bottom edges. At right top corner, a white beam emanates diagonally, oriented from 10 ou2019clock to 4 ou2019clock, from either side of a small, glowing, white star.
This artist’s concept shows what the exoplanet called PSR J2322-2650b (left) may look like as it orbits a rapidly spinning neutron star called a pulsar (right). Gravitational forces from the much heavier pulsar are pulling the Jupiter-mass world into a bizarre lemon shape.
Illustration: NASA, ESA, CSA, Ralf Crawford (STScI)

This planet-mass object was known to orbit a pulsar, a rapidly spinning neutron star. A pulsar emits beams of electromagnetic radiation at regular intervals typically ranging from milliseconds to seconds. These pulsing beams can only be seen when they are pointing directly toward Earth, much like beams from a lighthouse.  

This millisecond pulsar is expected to be emitting mostly gamma rays and other high energy particles, which are invisible to Webb’s infrared vision. Without a bright star in the way, scientists can study the planet in intricate detail across its whole orbit. 

“This system is unique because we are able to view the planet illuminated by its host star, but not see the host star at all,” said Maya Beleznay, a third-year PhD candidate at Stanford University in California who worked on modeling the shape of the planet and the geometry of its orbit. “So we get a really pristine spectrum. And we can study this system in more detail than normal exoplanets.” 

“The planet orbits a star that’s completely bizarre — the mass of the Sun, but the size of a city,” said the University of Chicago’s Michael Zhang, the principal investigator on this study. “This is a new type of planet atmosphere that nobody has ever seen before. Instead of finding the normal molecules we expect to see on an exoplanet — like water, methane, and carbon dioxide — we saw molecular carbon, specifically C3 and C2.”

Molecular carbon is very unusual because at these temperatures, if there are any other types of atoms in the atmosphere, carbon will bind to them. (Temperatures on the planet range from 1,200 degrees Fahrenheit at the coldest points of the night side to 3,700 degrees Fahrenheit at the hottest points of the day side.) Molecular carbon is only dominant if there’s almost no oxygen or nitrogen. Out of the approximately 150 planets that astronomers have studied inside and outside the solar system, no others have any detectable molecular carbon.

PSR J2322-2650b is extraordinarily close to its star, just 1 million miles away. In contrast, Earth’s distance from the Sun is about 100 million miles. Because of its extremely tight orbit, the exoplanet’s entire year — the time it takes to go around its star — is just 7.8 hours. Gravitational forces from the much heavier pulsar are pulling the Jupiter-mass planet into a bizarre lemon shape.

Image B: Exoplanet PSR J2322-2650b (Artist’s Concept)

Partially illuminated, lemon-shaped planet appears against a black background. The planet is most brightly illuminated at its elongated tip on its right side. On the left side, which is wider, the planet trails off into the darkness of the background. The planet is colored in varying, mottled shades of red, light pink, and fuchsia. Most of the pink occurs closest to the tip, while most of the fuchsia is at the top and bottom edges.
This artist’s concept shows what the exoplanet PSR J2322-2650b may look like. Gravitational forces from the much heavier pulsar it orbits are pulling the Jupiter-mass world into this bizarre lemon shape.
Illustration: NASA, ESA, CSA, Ralf Crawford (STScI)

Together, the star and exoplanet may be considered a “black widow” system, though not a typical example. Black widow systems are a rare type of double system where a rapidly spinning pulsar is paired with a small, low-mass stellar companion. In the past, material from the companion streamed onto the pulsar, causing the pulsar to spin faster over time, which powers a strong wind. That wind and radiation then bombard and evaporate the smaller and less massive companion. Like the spider for which it is named, the pulsar slowly consumes its unfortunate partner.

But in this case, the companion is officially considered an exoplanet, not a star. The International Astronomical Union defines an exoplanet as a celestial body below 13 Jupiter masses that orbits a star, brown dwarf, or stellar remnant, such as a pulsar.

Of the 6,000 known exoplanets, this is the only one reminiscent of a gas giant (with mass, radius, and temperature similar to a hot Jupiter) orbiting a pulsar. Only a handful of pulsars are known to have planets.

“Did this thing form like a normal planet? No, because the composition is entirely different,” said Zhang. “Did it form by stripping the outside of a star, like ‘normal’ black widow systems are formed? Probably not, because nuclear physics does not make pure carbon. It’s very hard to imagine how you get this extremely carbon-enriched composition. It seems to rule out every known formation mechanism.”

Study co-author Roger Romani, of Stanford University and the Kavli Institute for Particle Astrophysics and Cosmology Institute, proposes one evocative phenomenon that could occur in the unique atmosphere. “As the companion cools down, the mixture of carbon and oxygen in the interior starts to crystallize,” said Romani. “Pure carbon crystals float to the top and get mixed into the helium, and that’s what we see. But then something has to happen to keep the oxygen and nitrogen away. And that’s where the mystery come in.

“But it’s nice to not know everything,” said Romani. “I’m looking forward to learning more about the weirdness of this atmosphere. It’s great to have a puzzle to go after.”

Video A: Exoplanet PSR J2322-2650b and Pulsar (Artist’s Concept)

This animation shows an exotic exoplanet orbiting a distant pulsar, or rapidly rotating neutron star with radio pulses. The planet, which orbits about 1 million miles away from the pulsar, is stretched into a lemon shape by the pulsar’s strong gravitational tides.

Animation: NASA, ESA, CSA, Ralf Crawford (STScI)

With its infrared vision and exquisite sensitivity, this is a discovery only the Webb telescope could make. Its perch a million miles from Earth and its huge sunshield keep the instruments very cold, which is necessary for these observations. It is not possible to conduct this study from the ground.

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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Related Images & Videos

llustration labeled u201cartistu2019s conceptu201d at right bottom corner. At left bottom corner, a partially illuminated, lemon-shaped exoplanet appears against a black background. This planet is most brightly illuminated at its elongated tip on its right side. On the left side, which is wider, the planet trails off into the darkness of the background. The planet is colored in varying, mottled shades of red, light pink, and fuchsia. Most of the pink occurs closest to the tip, while most of the fuchsia is at the top and bottom edges. At right top corner, a white beam emanates diagonally, oriented from 10 ou2019clock to 4 ou2019clock, from either side of a small, glowing, white star.

Exoplanet PSR J2322-2650b and Pulsar (Artist’s Concept)

This artist’s concept shows what the exoplanet called PSR J2322-2650b (left) may look like as it orbits a rapidly spinning neutron star called a pulsar (right). Gravitational forces from the much heavier pulsar are pulling the Jupiter-mass world into a bizarre lemon shape.

Partially illuminated, lemon-shaped planet appears against a black background. The planet is most brightly illuminated at its elongated tip on its right side. On the left side, which is wider, the planet trails off into the darkness of the background. The planet is colored in varying, mottled shades of red, light pink, and fuchsia. Most of the pink occurs closest to the tip, while most of the fuchsia is at the top and bottom edges.

Exoplanet PSR J2322-2650b (Artist’s Concept)

This artist’s concept shows what the exoplanet PSR J2322-2650b may look like. Gravitational forces from the much heavier pulsar it orbits are pulling the Jupiter-mass world into this bizarre lemon shape.

Against a black background, a white beam emanates diagonally, oriented from 11 ou2019clock to 5 ou2019clock, from either side of a small, glowing, white star. To the right of this star, a partially illuminated, lemon-shaped exoplanet appears. This planet is most brightly illuminated at its elongated tip on its left side. The planetu2019s right side, which is wider, appears to trail off into the darkness of the background. The planet is colored in varying, mottled shades of red, light pink, and fuchsia. Most of the pink occurs closest to the tip, while most of the fuchsia is at the top and bottom edges.

Exoplanet PSR J2322-2650b Orbiting a Pulsar

This animation shows an exotic exoplanet orbiting a distant pulsar, or rapidly rotating neutron star with radio pulses. The planet, which orbits about 1 million miles away from the pulsar, is stretched into a lemon shape by the pulsar’s strong gravitational tides. NASA&rsqu…

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Dec 16, 2025

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Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov

Ann Jenkins
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Baltimore, Maryland

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Baltimore, Maryland

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NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame

NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame
NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame
NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame
NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame
NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame
NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame
NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame
NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame
NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame
NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame
NASA’s Webb, Curiosity Named in TIME’s Best Inventions Hall of Fame
Image composited from an image of Curiosity in a rocky Mars landscape and Webb Telescope over a star filled background
NASA’s James Webb Space Telescope and NASA’s Curiosity rover, have earned places in TIME’s “Best Inventions Hall of Fame”.
NASA GSFC, NASA JPL

Two icons of discovery, NASA’s James Webb Space Telescope and NASA’s Curiosity rover, have earned places in TIME’s “Best Inventions Hall of Fame,” which recognizes the 25 groundbreaking inventions of the past quarter century that have had the most global impact, since TIME began its annual Best Inventions list in 2000. The inventions are celebrated in TIME’s December print issue.

“NASA does the impossible every day, and it starts with the visionary science that propels humanity farther than ever before,” said Nicky Fox, associate administrator, Science Mission Directorate, NASA Headquarters in Washington. “Congratulations to the teams who made the world’s great engineering feats, the James Webb Space Telescope and the Mars Curiosity Rover, a reality. Through their work, distant galaxies feel closer, and the red sands of Mars are more familiar, as they expanded and redefined the bounds of human achievement in the cosmos for the benefit of all.”

Decades in the making and operating a million miles from Earth, Webb is the most powerful space telescope ever built, giving humanity breathtaking views of newborn stars, distant galaxies, and even planets orbiting other stars. The new technologies developed to enable Webb’s science goals – from optics to detectors to thermal control systems – now also touch Americans’ everyday lives, improving manufacturing for everything from high-end cameras and contact lenses to advanced semiconductors and inspections of aircraft engine components.

This landscape of “mountains” and “valleys” speckled with glittering stars is actually the edge of a nearby, young, star-forming region called NGC 3324 in the Carina Nebula. Captured in infrared light by NASA’s James Webb Space Telescope, this image reveals for the first time previously invisible areas of star birth.
NASA, ESA, CSA, and STScI

Meanwhile on Mars, the unstoppable Curiosity rover, NASA’s car-size science lab, has spent more than a decade uncovering clues that the Red Planet once could have supported life, transforming our understanding of our planetary neighbor. These NASA missions continue to make breakthroughs that have reshaped our understanding of the universe and our place in it. Curiosity has also paved the way for future astronauts: Its Radiation Assessment Detector has studied the Martian radiation environment for nearly 14 years, and its unforgettable landing by robotic jetpack allowed heavier spacecraft to touch down on the surface — a capability that will be needed to send cargo and humans to Mars.

Mars rover sitting on the red soil of mars and facing the camera for a selfie
NASA’s Curiosity Mars rover used two different cameras to create this selfie in front of Mont Mercou, a rock outcrop that stands 20 feet (6 meters) tall. The panorama is made up of 60 images taken by the Mars Hand Lens Imager (MAHLI) on the rover’s robotic arm on March 26, 2021, the 3,070th Martian day, or sol, of the mission. These were combined with 11 images taken by the Mastcam on the mast, or “head,” of the rover on March 16, 2021, the 3,060th Martian day of the mission.
NASA/JPL-Caltech/MSSS

To compile this “Hall of Fame” list, TIME solicited nominations from TIME editors and correspondents around the world, paying special attention to high-impact fields, such as health care and technology. TIME then evaluated each contender on a number of key factors, including originality, continued efficacy, ambition, and impact.

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).

The Curiosity rover was built by NASA’s Jet Propulsion Laboratory, which is managed by Caltech in Pasadena, California. JPL leads the mission on behalf of NASA’s Science Mission Directorate in Washington as part of NASA’s Mars Exploration Program portfolio.

To learn more about NASA’s science missions, visit:

https://science.nasa.gov

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NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 

NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 

 
6 Min Read

NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 

Illustration of a planet orbiting a star, with the words “Artist’s Concept” in the lower right corner.

This artist’s concept shows what the hot super-Earth exoplanet TOI-561 b and its star could look like based on observations from NASA’s James Webb Space Telescope and other observatories. Webb data suggests that the planet is surrounded by a thick atmosphere above a magma ocean.

Credits:
Illustration: NASA, ESA, CSA, Ralf Crawford (STScI)

Researchers using NASA’s James Webb Space Telescope have detected the strongest evidence yet for an atmosphere on a rocky planet outside our solar system, as NASA leads the world in exploring the universe from the Moon to Mars and beyond. Observations of the ultra-hot super-Earth TOI-561 b suggest that the exoplanet is surrounded by a thick blanket of gases above a global magma ocean. The results help explain the planet’s unusually low density and challenge the prevailing wisdom that relatively small planets so close to their stars are not able to sustain atmospheres.  

Image A: Super-Earth Exoplanet TOI-561 b and Its Star (Artist’s Concept)

Illustration of a planet orbiting a star, with the words u201cArtistu2019s Conceptu201d in the lower right corner.
This artist’s concept shows what the hot super-Earth exoplanet TOI-561 b and its star could look like based on observations from NASA’s James Webb Space Telescope and other observatories. Webb data suggests that the planet is surrounded by a thick atmosphere above a magma ocean.
Illustration: NASA, ESA, CSA, Ralf Crawford (STScI)

With a radius roughly 1.4 times Earth’s, and an orbital period less than 11 hours, TOI-561 b falls into a rare class of objects known as ultra-short period exoplanets. Although its host star is only slightly smaller and cooler than the Sun, TOI-561 b orbits so close to the star — less than one million miles (one-fortieth the distance between Mercury and the Sun) — that it must be tidally locked, with the temperature of its permanent dayside far exceeding the melting temperature of typical rock.

“What really sets this planet apart is its anomalously low density,” said  Johanna Teske, staff scientist at Carnegie Science Earth and Planets Laboratory and lead author on a paper published Thursday in The Astrophysical Journal Letters. “It’s not a super-puff, but it is less dense than you would expect if it had an Earth-like composition.”

Image B: Super-Earth Exoplanet TOI-561 b (Artist’s Concept)

Illustration showing a planet that appears to have a partially molten surface and a thick atmosphere.
An artist’s concept shows what a thick atmosphere above a vast magma ocean on exoplanet TOI-561 b could look like. Measurements captured by NASA’s James Webb Space Telescope suggest that in spite of the intense radiation it receives from its star, TOI-561 b is not a bare rock.
Illustration: NASA, ESA, CSA, Ralf Crawford (STScI)

One explanation the team considered for the planet’s low density was that it could have a relatively small iron core and a mantle made of rock that is not as dense as rock within Earth. Teske notes that this could make sense: “TOI-561 b is distinct among ultra-short period planets in that it orbits a very old (twice as old as the Sun), iron-poor star in a region of the Milky Way known as the thick disk. It must have formed in a very different chemical environment from the planets in our own solar system.” The planet’s composition could be representative of planets that formed when the universe was relatively young. 

But an exotic composition can’t explain everything. The team also suspected that TOI-561 b might be surrounded by a thick atmosphere that makes it look larger than it actually is. Although small planets that have spent billions of years baking in blazing stellar radiation are not expected to have atmospheres, some show signs that they are not just bare rock or lava. 

To test the hypothesis that TOI-561 b has an atmosphere, the team used Webb’s NIRSpec (Near-Infrared Spectrograph) to measure the planet’s dayside temperature based on its near-infrared brightness. The technique, which involves measuring the decrease in brightness of the star-planet system as the planet moves behind the star, is similar to that used to search for atmospheres in the TRAPPIST-1 system and on other rocky worlds. 

If TOI-561 b is a bare rock with no atmosphere to carry heat around to the nightside, its dayside temperature should be approaching 4,900 degrees Fahrenheit (2,700 degrees Celsius). But the NIRSpec observations show that the planet’s dayside appears to be closer to 3,200 degrees Fahrenheit (1,800 degrees Celsius) — still extremely hot, but far cooler than expected. 

Image C: Super-Earth Exoplanet TOI-561 b (NIRSpec Emission Spectrum)

Infographic titled “Hot Lava World TOI-561 b: Secondary Eclipse Emission Spectrum; NIRSpec Bright Object time-Series Spectroscopy (G395H)” showing a graph of brightness versus wavelength, with one set of data and three model spectra.
An emission spectrum captured by NASA’s James Webb Space Telescope in May 2024 shows the brightness of different wavelengths of near-infrared light emitted by exoplanet TOI-561 b. Comparing the data to models suggests that the planet is surrounded by a volatile-rich atmosphere.
Illustration: NASA, ESA, CSA, Ralf Crawford (STScI); Science: Johanna Teske (Carnegie Science Earth and Planets Laboratory), Anjali Piette (University of Birmingham), Tim Lichtenberg (Groningen), Nicole Wallack (Carnegie Science Earth and Planets Laboratory)

To explain the results, the team considered a few different scenarios. The magma ocean could circulate some heat, but without an atmosphere, the nightside would probably be solid, limiting flow away from the dayside. A thin layer of rock vapor on the surface of the magma ocean is also possible, but on its own would likely have a much smaller cooling effect than observed. 

“We really need a thick volatile-rich atmosphere to explain all the observations,” said Anjali Piette, coauthor from the University of Birmingham, United Kingdom. 

“Strong winds would cool the dayside by transporting heat over to the nightside. Gases like water vapor would absorb some wavelengths of near-infrared light emitted by the surface before they make it all the way up through the atmosphere. (The planet would look colder because the telescope detects less light.) It’s also possible that there are bright silicate clouds that cool the atmosphere by reflecting starlight.”

While the Webb observations provide compelling evidence for such an atmosphere, the question remains: How can a small planet exposed to such intense radiation can hold on to any atmosphere at all, let alone one so substantial? Some gases must be escaping to space, but perhaps not as efficiently as expected. 

“We think there is an equilibrium between the magma ocean and the atmosphere. At the same time that gases are coming out of the planet to feed the atmosphere, the magma ocean is sucking them back into the interior,” said co-author Tim Lichtenberg from the University of Groningen in the Netherlands. “This planet must be much, much more volatile-rich than Earth to explain the observations. It’s really like a wet lava ball.”

These are the first results from Webb’s General Observers Program 3860, which involved observing the system continuously for more than 37 hours while TOI-561 b completed nearly four full orbits of the star. The team is currently analyzing the full data set to map the temperature all the way around the planet and narrow down the composition of the atmosphere.  

“What’s really exciting is that this new data set is opening up even more questions than it’s answering,” said Teske. 

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

Read more: Can Rocky Worlds Orbiting Red Dwarf Stars Maintain Atmospheres?

Explore more: ViewSpace Exoplanet Variety: Atmosphere

Explore more: How to Study Exoplanets: Webb and Challenges

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Related Images & Videos

Illustration of a planet orbiting a star, with the words u201cArtistu2019s Conceptu201d in the lower right corner.

Super-Earth Exoplanet TOI-561 b and Its Star (Artist’s Concept)

This artist’s concept shows what the hot super-Earth exoplanet TOI-561 b and its star could look like based on observations from NASA’s James Webb Space Telescope and other observatories. Webb data suggests that the planet is surrounded by a thick atmosphere above a magma ocean.

Illustration showing a planet that appears to have a partially molten surface and a thick atmosphere.

Super-Earth Exoplanet TOI-561 b (Artist’s Concept)

An artist’s concept shows what a thick atmosphere above a vast magma ocean on exoplanet TOI-561 b could look like. Measurements captured by NASA’s James Webb Space Telescope suggest that in spite of the intense radiation it receives from its star, TOI-561 b is not a bare rock.

Infographic titled u201cHot Lava World TOI-561 b: Secondary Eclipse Emission Spectrum; NIRSpec Bright Object time-Series Spectroscopy (G395H)u201d showing a graph of brightness versus wavelength, with one set of data and three model spectra.

Super-Earth Exoplanet TOI-561 b (NIRSpec Emission Spectrum)

An emission spectrum captured by NASA’s James Webb Space Telescope in May 2024 shows the brightness of different wavelengths of near-infrared light emitted by exoplanet TOI-561 b. Comparing the data to models suggests that the planet is surrounded by a volatile-rich atmosphere.

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Dec 12, 2025

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Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov

Margaret Carruthers
Space Telescope Science Institute
Baltimore, Maryland

Hannah Braun
Space Telescope Science Institute
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Source Link NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World 

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NASA’s Chandra Finds Small Galaxies May Buck the Black Hole Trend

NASA’s Chandra Finds Small Galaxies May Buck the Black Hole Trend
NASA’s Chandra Finds Small Galaxies May Buck the Black Hole Trend
NASA’s Chandra Finds Small Galaxies May Buck the Black Hole Trend
NASA’s Chandra Finds Small Galaxies May Buck the Black Hole Trend
NASA’s Chandra Finds Small Galaxies May Buck the Black Hole Trend
NGC 6278 and PGC 039620 are two galaxies from a sample of 1,600 that were searched for the presence of supermassive black holes. These images represent the results of a study that suggests that smaller galaxies do not contain supermassive black holes nearly as often as larger galaxies do. The study analyzed over 1,600 galaxies that have been observed with Chandra over two decades. Certain X-ray signatures indicate the presence of supermassive black holes. The study indicates that most smaller galaxies like PGC 03620, shown here in both X-rays from Chandra and optical light images from the Sloan Digital Sky Survey, likely do not have supermassive black holes in their centers. In contrast, NGC 6278, which is roughly the same size as the Milky Way, and most other large galaxies in the sample show evidence for giant black holes within their cores.
NGC 6278 and PGC 039620 are two galaxies from a sample of 1,600 that were searched for the presence of supermassive black holes. These images represent the results of a study that suggests that smaller galaxies do not contain supermassive black holes nearly as often as larger galaxies do. The study analyzed over 1,600 galaxies that have been observed with Chandra over two decades. Certain X-ray signatures indicate the presence of supermassive black holes. The study indicates that most smaller galaxies like PGC 03620, shown here in both X-rays from Chandra and optical light images from the Sloan Digital Sky Survey, likely do not have supermassive black holes in their centers. In contrast, NGC 6278, which is roughly the same size as the Milky Way, and most other large galaxies in the sample show evidence for giant black holes within their cores.
X-ray: NASA/CXC/SAO/F. Zou et al.; Optical: SDSS; Image Processing: NASA/CXC/SAO/N. Wolk

Most smaller galaxies may not have supermassive black holes in their centers, according to a recent  study using NASA’s Chandra X-ray Observatory. This contrasts with the common idea that nearly every galaxy has one of these giant black holes within their cores, as NASA leads the world in exploring how our universe works.

A team of astronomers used data from over 1,600 galaxies collected in more than two decades of the Chandra mission. The researchers looked at galaxies ranging in heft from over ten times the mass of the Milky Way down to dwarf galaxies, which have stellar masses less than a few percent of that of our home galaxy. A paper describing these results has been published in The Astrophysical Journal and is available here https://arxiv.org/abs/2510.05252. 

The team has reported that only about 30% of dwarf galaxies likely contain supermassive black holes.

“It’s important to get an accurate black hole head count in these smaller galaxies,” said Fan Zou of the University of Michigan in Ann Arbor, who led the study. “It’s more than just bookkeeping. Our study gives clues about how supermassive black holes are born. It also provides crucial hints about how often black hole signatures in dwarf galaxies can be found with new or future telescopes.”

As material falls onto black holes, it is heated by friction and produces X-rays. Many of the massive galaxies in the study contain bright X-ray sources in their centers, a clear signature of supermassive black holes in their centers. The team concluded that more than 90% of massive galaxies – including those with the mass of the Milky Way – contain supermassive black holes.

However, smaller galaxies in the study usually did not have these unambiguous black hole signals. Galaxies with masses less than three billion Suns – about the mass of the Large Magellanic Cloud, a close neighbor to the Milky Way – usually do not contain bright X-ray sources in their centers.

The researchers considered two possible explanations for this lack of X-ray sources. The first is that the fraction of galaxies containing massive black holes is much lower for these less massive galaxies. The second is the amount of X-rays produced by matter falling onto these black holes is so faint that Chandra cannot detect it.

“We think, based on our analysis of the Chandra data, that there really are fewer black holes in these smaller galaxies than in their larger counterparts,” said Elena Gallo, a co-author also from the University of Michigan.

To reach their conclusion, Zou and his colleagues considered both possibilities for the lack of X-ray sources in small galaxies in their large Chandra sample. The amount of gas falling onto a black hole determines how bright or faint they are in X-rays. Because smaller black holes are expected to pull in less gas than larger black holes, they should be fainter in X-rays and often not detectable. The researchers confirmed this expectation. 

However, they found that an additional deficit of X-ray sources is seen in less massive galaxies beyond the expected decline from decreases in the amount of gas falling inwards. This additional deficit can be accounted for if many of the low-mass galaxies simply don’t have any black holes at their centers. The team’s conclusion was that the drop in X-ray detections in lower mass galaxies reflects a true decrease in the number of black holes located in these galaxies.

This result could have important implications for understanding how supermassive black holes form. There are two main ideas: In the first, a giant gas cloud directly collapses into a black hole, which contains thousands of times the Sun’s mass from the start. The other idea is that supermassive black holes instead come from much smaller black holes, created when massive stars collapse.

“The formation of big black holes is expected to be rarer, in the sense that it occurs preferentially in the most massive galaxies being formed, so that would explain why we don’t find black holes in all the smaller galaxies,” said co-author Anil Seth of the University of Utah.

This study supports the theory where giant black holes are born already weighing several thousand times the Sun’s mass. If the other idea were true, the researchers said they would have expected smaller galaxies to likely have the same fraction of black holes as larger ones.

This result also could have important implications for the rates of black hole mergers from the collisions of dwarf galaxies. A much lower number of black holes would result in fewer sources of gravitational waves to be detected in the future by the Laser Interferometer Space Antenna. The number of black holes tearing stars apart in dwarf galaxies will also be smaller.

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.

To learn more about Chandra, visit:

https://science.nasa.gov/chandra


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Megan Watzke
Chandra X-ray Center
Cambridge, Mass.
617-496-7998
mwatzke@cfa.harvard.edu

Corinne Beckinger
Marshall Space Flight Center, Huntsville, Alabama
256-544-0034
corinne.m.beckinger@nasa.gov

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Dec 11, 2025

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Lee Mohon
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Source Link NASA’s Chandra Finds Small Galaxies May Buck the Black Hole Trend

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Massive Stars Make Their Mark in Hubble Image

Massive Stars Make Their Mark in Hubble Image
Massive Stars Make Their Mark in Hubble Image
Massive Stars Make Their Mark in Hubble Image
Massive Stars Make Their Mark in Hubble Image
Massive Stars Make Their Mark in Hubble Image
Massive Stars Make Their Mark in Hubble Image
Massive Stars Make Their Mark in Hubble Image
Massive Stars Make Their Mark in Hubble Image
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Massive Stars Make Their Mark in Hubble Image

A pale blue dwarf galaxy on the black backdrop of space with some faraway galaxies. The galaxy itself resembles a fuzzy cloud of tightly packed stars, with a broad halo of stars dispersed around it. Spread across the galaxy’s core are several small, glowing patches of gas where there is a concentration of very hot stars.
This NASA/ESA Hubble Space Telescope image features the blue dwarf galaxy Markarian 178 (Mrk 178) against a backdrop of distant galaxies in all shapes and sizes. Some of these distant galaxies even shine through the diffuse edges of Mrk 178.
ESA/Hubble & NASA, F. Annibali, S. Hong

This NASA/ESA Hubble Space Telescope image features a glittering blue dwarf galaxy called Markarian 178 (Mrk 178). The galaxy, which is substantially smaller than our own Milky Way, lies 13 million light-years away in the constellation Ursa Major (the Great Bear).

Mrk 178 is one of more than 1,500 Markarian galaxies. These galaxies get their name from the Armenian astrophysicist Benjamin Markarian, who compiled a list of galaxies that were surprisingly bright in ultraviolet light.

While the bulk of the galaxy is blue due to an abundance of young, hot stars with little dust shrouding them, Mrk 178 gets a red hue from a collection of rare massive Wolf–Rayet stars. These stars are concentrated in the brightest, reddish region near the galaxy’s edge. Wolf–Rayet stars cast off their atmospheres through powerful winds, and the bright emission lines from their hot stellar winds are etched upon the galaxy’s spectrum. Both ionized hydrogen and oxygen lines are particularly strong and appear as a red color in this photo.

Massive stars enter the Wolf–Rayet phase of their evolution just before they collapse into black holes or neutron stars. Because Wolf–Rayet stars last for only a few million years, researchers know that something must have triggered a recent burst of star formation in Mrk 178. At first glance, it’s not clear what could be the cause — Mrk 178 doesn’t seem to have any close galactic neighbors that may have stirred up its gas to form new stars. Instead, researchers suspect that a gas cloud crashed into Mrk 178, or that the intergalactic medium disturbed its gas as the galaxy moved through space. Either disturbance could light up this tiny galaxy with a ripple of bright new stars.

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Claire Andreoli (claire.andreoli@nasa.gov)
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Dec 11, 2025

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Source Link Massive Stars Make Their Mark in Hubble Image

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