Feed aggregator
Disney and OpenAI have made a surprise deal – what happens next?
U.S. Sunscreens Aren’t Great. The FDA Could Soon Change That
The U.S. is considering allowing bemotrizinol, a highly effective UV filter used throughout Europe and Asia, in its sunscreen products for the first time
Two Stars Swept by the Solar System 4.5 Million Years Ago
Two winter stars left their mark long ago on wispy gas clouds near the solar system. Their passage might even have influenced life on Earth.
The post Two Stars Swept by the Solar System 4.5 Million Years Ago appeared first on Sky & Telescope.
Measles Outbreaks Accelerate as U.S. Inches Closer to a Disease Tipping Point
More than 1,900 people, mostly children, have been sickened by measles in the U.S. in 2025. The outbreaks are moving the country toward losing its measles-free status by early next year
Killer Whales and Dolphins May Team Up to Hunt Salmon
Tantalizing observations suggest marine mammals may be teaming up to hunt
NASA’s Parker Solar Probe Spies Solar Wind ‘U-Turn’
5 min read
NASA’s Parker Solar Probe Spies Solar Wind ‘U-Turn’Images captured by NASA’s Parker Solar Probe as the spacecraft made its record-breaking closest approach to the Sun in December 2024 have now revealed new details about how solar magnetic fields responsible for space weather escape from the Sun — and how sometimes they don’t.
Like a toddler, our Sun occasionally has disruptive outbursts. But instead of throwing a fit, the Sun spews magnetized material and hazardous high-energy particles that drive space weather as they travel across the solar system. These outbursts can impact our daily lives, from disrupting technologies like GPS to triggering power outages, and they can also imperil voyaging astronauts and spacecraft. Understanding how these solar outbursts, called coronal mass ejections (CMEs), occur and where they are headed is essential to predicting and preparing for their impacts at Earth, the Moon, and Mars.
Images taken by Parker Solar Probe in December 2024, and published Thursday in the Astrophysical Journal Letters, have revealed that not all magnetic material in a CME escapes the Sun — some makes it back, changing the shape of the solar atmosphere in subtle, but significant, ways that can set the course of the next CME exploding from the Sun. These findings have far-reaching implications for understanding how the CME-driven release of magnetic fields affects not only the planets, but the Sun itself.
To view this video please enable JavaScript, and consider upgrading to a web browser that
supports HTML5 video
“These breathtaking images are some of the closest ever taken to the Sun and they’re expanding what we know about our closest star,” said Joe Westlake, heliophysics division director at NASA Headquarters in Washington. “The insights we gain from these images are an important part of understanding and predicting how space weather moves through the solar system, especially for mission planning that ensures the safety of our Artemis astronauts traveling beyond the protective shield of our atmosphere.”
Parker Solar Probe reveals solar recycling in actionAs Parker Solar Probe swept through the Sun’s atmosphere on Dec. 24, 2024, just 3.8 million miles from the solar surface, its Wide-Field Imager for Solar Probe, or WISPR, observed a CME erupt from the Sun. In the CME’s wake, elongated blobs of solar material were seen falling back toward the Sun.
This type of feature, called “inflows”, has previously been seen from a distance by other NASA missions including SOHO (Solar and Heliospheric Observatory, a joint mission with ESA, the European Space Agency) and STEREO (Solar Terrestrial Relations Observatory). But Parker Solar Probe’s extreme close-up view from within the solar atmosphere reveals details of material falling back toward the Sun and on scales never seen before.
“We’ve previously seen hints that material can fall back into the Sun this way, but to see it with this clarity is amazing,” said Nour Rawafi, the project scientist for Parker Solar Probe at the Johns Hopkins Applied Physics Laboratory, which designed, built, and operates the spacecraft in Laurel, Maryland. “This is a really fascinating, eye-opening glimpse into how the Sun continuously recycles its coronal magnetic fields and material.”
Insights on inflowsFor the first time, the high-resolution images from Parker Solar Probe allowed scientists to make precise measurements about the inflow process, such as the speed and size of the blobs of material pulled back into the Sun. These previously hidden details provide scientists with new insights into the physical mechanisms that reconfigure the solar atmosphere.
1. The process that creates inflows begins with a solar eruption known as a coronal mass ejection (CME). CMEs are often triggered by twisted magnetic field lines from the Sun that explosively snap and realign in a process called magnetic reconnection. This magnetic explosion kicks out a burst of charged particles and magnetic fields — the CME. NASA 2.As the CME travels outward from the Sun, the CME expands. Eventually, it pushes through solar magnetic field lines to escape into space. NASA 3. The magnetic field lines torn open by the CME rejoin to form new magnetic loops that get squeezed together. NASA 4. In some cases, the compressed magnetic field lines tear apart. This forms separate magnetic loops, some of which travel outward from the Sun and others that connect back to the Sun. As these loops contract back into the Sun, they drag down blobs of nearby solar material — forming inflows. NASAThe CMEs are often triggered by twisted magnetic field lines that explosively snap and realign in a process called magnetic reconnection. This magnetic explosion kicks out a burst of charged particles and magnetic fields — a CME.
As the CME travels outward from the Sun, it expands, in some cases causing nearby magnetic field lines to tear apart like the threads of an old piece of cloth pulled too tight. The torn magnetic field quickly mends itself, creating separate magnetic loops. Some of the loops travel outward from the Sun, and others stitch back to the Sun, forming inflows.
“It turns out, some of the magnetic field released with the CME does not escape as we would expect,” said Angelos Vourlidas, WISPR project scientist and researcher at Johns Hopkins Applied Physics Laboratory. “It actually lingers for a while and eventually returns to the Sun to be recycled, reshaping the solar atmosphere in subtle ways.”
An important result of this magnetic recycling is that as the inflows contract back into the Sun, they drag down blobs of nearby solar material and ultimately affect the magnetic fields swirling beneath. This interaction reconfigures the solar magnetic landscape, potentially altering the trajectories of subsequent CMEs that may emerge from the region.
“The magnetic reconfiguration caused by inflows may be enough to point a secondary CME a few degrees in a different direction,” Vourlidas said. “That’s enough to be the difference between a CME crashing into Mars versus sweeping by the planet with no or little effects.”
Scientists are using the new findings to improve their models of space weather and the Sun’s complex magnetic environment. Ultimately, this work may help scientists better predict the impact of space weather across the solar system on longer timescales than currently possible.
“Eventually, with more and more passes by the Sun, Parker Solar Probe will help us be able to continue building the big picture of the Sun’s magnetic fields and how they can affect us,” Rawafi said. “And as the Sun transitions from solar maximum toward minimum, the scenes we’ll witness may be even more dramatic.”
By Mara Johnson-Groh
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Article
3 hours ago
2 min read Massive Stars Make Their Mark in Hubble Image
Article
9 hours ago
3 min read Pacific Moisture Drenches the U.S. Northwest
A potent atmospheric river delivered intense rainfall to western Washington, triggering flooding and mudslides.
Article
16 hours ago
Keep Exploring Discover More Topics From NASA
Missions
Humans in Space
Climate Change
Solar System
NASA’s Parker Solar Probe Spies Solar Wind ‘U-Turn’
5 min read
NASA’s Parker Solar Probe Spies Solar Wind ‘U-Turn’Images captured by NASA’s Parker Solar Probe as the spacecraft made its record-breaking closest approach to the Sun in December 2024 have now revealed new details about how solar magnetic fields responsible for space weather escape from the Sun — and how sometimes they don’t.
Like a toddler, our Sun occasionally has disruptive outbursts. But instead of throwing a fit, the Sun spews magnetized material and hazardous high-energy particles that drive space weather as they travel across the solar system. These outbursts can impact our daily lives, from disrupting technologies like GPS to triggering power outages, and they can also imperil voyaging astronauts and spacecraft. Understanding how these solar outbursts, called coronal mass ejections (CMEs), occur and where they are headed is essential to predicting and preparing for their impacts at Earth, the Moon, and Mars.
Images taken by Parker Solar Probe in December 2024, and published Thursday in the Astrophysical Journal Letters, have revealed that not all magnetic material in a CME escapes the Sun — some makes it back, changing the shape of the solar atmosphere in subtle, but significant, ways that can set the course of the next CME exploding from the Sun. These findings have far-reaching implications for understanding how the CME-driven release of magnetic fields affects not only the planets, but the Sun itself.
To view this video please enable JavaScript, and consider upgrading to a web browser that
supports HTML5 video
“These breathtaking images are some of the closest ever taken to the Sun and they’re expanding what we know about our closest star,” said Joe Westlake, heliophysics division director at NASA Headquarters in Washington. “The insights we gain from these images are an important part of understanding and predicting how space weather moves through the solar system, especially for mission planning that ensures the safety of our Artemis astronauts traveling beyond the protective shield of our atmosphere.”
Parker Solar Probe reveals solar recycling in actionAs Parker Solar Probe swept through the Sun’s atmosphere on Dec. 24, 2024, just 3.8 million miles from the solar surface, its Wide-Field Imager for Solar Probe, or WISPR, observed a CME erupt from the Sun. In the CME’s wake, elongated blobs of solar material were seen falling back toward the Sun.
This type of feature, called “inflows”, has previously been seen from a distance by other NASA missions including SOHO (Solar and Heliospheric Observatory, a joint mission with ESA, the European Space Agency) and STEREO (Solar Terrestrial Relations Observatory). But Parker Solar Probe’s extreme close-up view from within the solar atmosphere reveals details of material falling back toward the Sun and on scales never seen before.
“We’ve previously seen hints that material can fall back into the Sun this way, but to see it with this clarity is amazing,” said Nour Rawafi, the project scientist for Parker Solar Probe at the Johns Hopkins Applied Physics Laboratory, which designed, built, and operates the spacecraft in Laurel, Maryland. “This is a really fascinating, eye-opening glimpse into how the Sun continuously recycles its coronal magnetic fields and material.”
Insights on inflowsFor the first time, the high-resolution images from Parker Solar Probe allowed scientists to make precise measurements about the inflow process, such as the speed and size of the blobs of material pulled back into the Sun. These previously hidden details provide scientists with new insights into the physical mechanisms that reconfigure the solar atmosphere.
1. The process that creates inflows begins with a solar eruption known as a coronal mass ejection (CME). CMEs are often triggered by twisted magnetic field lines from the Sun that explosively snap and realign in a process called magnetic reconnection. This magnetic explosion kicks out a burst of charged particles and magnetic fields — the CME. NASA 2.As the CME travels outward from the Sun, the CME expands. Eventually, it pushes through solar magnetic field lines to escape into space. NASA 3. The magnetic field lines torn open by the CME rejoin to form new magnetic loops that get squeezed together. NASA 4. In some cases, the compressed magnetic field lines tear apart. This forms separate magnetic loops, some of which travel outward from the Sun and others that connect back to the Sun. As these loops contract back into the Sun, they drag down blobs of nearby solar material — forming inflows. NASAThe CMEs are often triggered by twisted magnetic field lines that explosively snap and realign in a process called magnetic reconnection. This magnetic explosion kicks out a burst of charged particles and magnetic fields — a CME.
As the CME travels outward from the Sun, it expands, in some cases causing nearby magnetic field lines to tear apart like the threads of an old piece of cloth pulled too tight. The torn magnetic field quickly mends itself, creating separate magnetic loops. Some of the loops travel outward from the Sun, and others stitch back to the Sun, forming inflows.
“It turns out, some of the magnetic field released with the CME does not escape as we would expect,” said Angelos Vourlidas, WISPR project scientist and researcher at Johns Hopkins Applied Physics Laboratory. “It actually lingers for a while and eventually returns to the Sun to be recycled, reshaping the solar atmosphere in subtle ways.”
An important result of this magnetic recycling is that as the inflows contract back into the Sun, they drag down blobs of nearby solar material and ultimately affect the magnetic fields swirling beneath. This interaction reconfigures the solar magnetic landscape, potentially altering the trajectories of subsequent CMEs that may emerge from the region.
“The magnetic reconfiguration caused by inflows may be enough to point a secondary CME a few degrees in a different direction,” Vourlidas said. “That’s enough to be the difference between a CME crashing into Mars versus sweeping by the planet with no or little effects.”
Scientists are using the new findings to improve their models of space weather and the Sun’s complex magnetic environment. Ultimately, this work may help scientists better predict the impact of space weather across the solar system on longer timescales than currently possible.
“Eventually, with more and more passes by the Sun, Parker Solar Probe will help us be able to continue building the big picture of the Sun’s magnetic fields and how they can affect us,” Rawafi said. “And as the Sun transitions from solar maximum toward minimum, the scenes we’ll witness may be even more dramatic.”
By Mara Johnson-Groh
NASA’s Goddard Space Flight Center, Greenbelt, Md.
Article
3 hours ago
2 min read Massive Stars Make Their Mark in Hubble Image
Article
9 hours ago
3 min read Pacific Moisture Drenches the U.S. Northwest
A potent atmospheric river delivered intense rainfall to western Washington, triggering flooding and mudslides.
Article
16 hours ago
Keep Exploring Discover More Topics From NASA
Missions
Humans in Space
Climate Change
Solar System
Killer whales and dolphins are ‘being friends’ to hunt salmon together
Killer whales and dolphins are ‘being friends’ to hunt salmon together
Stellar Jet
Stellar Jet
NASA’s James Webb Space Telescope captured a blowtorch of seething gasses erupting from a volcanically growing monster star in this image released on Sept. 10, 2025. Stellar jets, which are powered by the gravitational energy released as a star grows in mass, encode the formation history of the protostar. This image provides evidence that protostellar jets scale with the mass of their parent stars—the more massive the stellar engine driving the plasma, the larger the resulting jet.
Image credit: NASA, ESA, CSA, STScI, Yu Cheng (NAOJ); Image Processing: Joseph DePasquale (STScI)
Stellar Jet
NASA’s James Webb Space Telescope captured a blowtorch of seething gasses erupting from a volcanically growing monster star in this image released on Sept. 10, 2025. Stellar jets, which are powered by the gravitational energy released as a star grows in mass, encode the formation history of the protostar. This image provides evidence that protostellar jets scale with the mass of their parent stars—the more massive the stellar engine driving the plasma, the larger the resulting jet.
Image credit: NASA, ESA, CSA, STScI, Yu Cheng (NAOJ); Image Processing: Joseph DePasquale (STScI)
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World
- Webb
- News
- Overview
- Science
- Observatory
- Multimedia
- Team
- More
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) 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) 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) 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:
Related InformationRead 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
Explore more: How Do We Learn About a Planet’s Atmosphere?
Read more: NASA’s Webb Hints at Possible Atmosphere Surrounding Rocky Exoplanet
Related For Kids Related Images & Videos 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.
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.
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.
Contact Media
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
Baltimore, Maryland
Related Terms Keep Exploring Related Topics James Webb Space Telescope
Space Telescope
Exoplanets
Exoplanet Stories
Universe
NASA’s Webb Detects Thick Atmosphere Around Broiling Lava World
- Webb
- News
- Overview
- Science
- Observatory
- Multimedia
- Team
- More
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) 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) 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) 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:
Related InformationRead 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
Explore more: How Do We Learn About a Planet’s Atmosphere?
Read more: NASA’s Webb Hints at Possible Atmosphere Surrounding Rocky Exoplanet
Related For Kids Related Images & Videos 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.
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.
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.
Contact Media
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
Baltimore, Maryland
Related Terms Keep Exploring Related Topics James Webb Space Telescope
Space Telescope
Exoplanets
Exoplanet Stories
Universe
Why 2025 is an Amazing Year to Catch the Geminid Meteors
It’s one of the better annual meteor showers, and 2025 is shaping up to give sky watchers a chance to see it at its best. If skies are clear this weekend, be sure to be vigilant for the Geminid meteors.
The Telescope That Will Study Our Nearest Exoplanet
Scientists at the University of Geneva have successfully tested key components of RISTRETTO, a new spectrograph designed to analyse light from Proxima b, the nearest exoplanet to Earth. The instrument uses coronagraphic techniques and extreme adaptive optics to block a star's overwhelming glare and detect planets that shine 10 million times fainter. Simulations suggest RISTRETTO could not only spot Proxima b with just 55 hours of observation time but potentially identify oxygen or water in its atmosphere, offering our first chance to study the conditions on an Earth sized world orbiting our nearest stellar neighbour.
A New Technique Reveals the Hidden Physics of the Universe's Giants
Astronomers have developed a new technique called "X-arithmetic" that reveals the hidden physics inside galaxy clusters. By analysing Chandra X-ray Observatory data at different energy levels and painting the results in vibrant colours, researchers can now distinguish between sound waves, black hole inflated bubbles, and cooling gas, enabling them to classify structures by what they are rather than how they look. The method has already exposed striking differences between galaxy clusters and galaxy groups, showing that supermassive black holes wield dramatically different influence on their surroundings.
The journey of Juice – episode 2
ESA’s Jupiter Icy Moons Explorer (Juice) is on an epic eight-year journey to Jupiter. It left Earth in April 2023 and is due to arrive at the gas giant in 2031.
2025 has been another big year for Juice. It made its closest approach to the Sun and flew close by Venus for a gravity boost to help it on its way. This second episode of ‘The journey of Juice’ takes us on a journey of our own, discovering what Juice – and the humans behind it – have experienced this year.
In a clean room at ESA’s technical centre, thermal engineer Romain Peyrou-Lauge shows us the technologies that protect Juice from the intense heat of the Sun during this period.
In Uppsala, Sweden, scientists get together for a ‘science working team’ meeting to discuss the scientific aspects of the mission. Juice Project Scientist Olivier Witasse talks about how important it is to continue working as a team to prepare for Juice’s precious time spent collecting data at Jupiter.
The video culminates with operations engineer Marc Costa taking us to the Cebreros station in Madrid for the Venus flyby. There we meet deputy station manager Jorge Fauste, Juice intern Charlotte Bergot and Juice Mission Manager Nicolas Altobelli.
This series follows on from ‘The making of Juice’ series, which covered the planning, testing and launch of this once-in-a-generation mission.
Reading the "Light Fingerprints" of Dead Satellites
There are already tens of thousands of pieces of large debris in orbit, some of which pose a threat to functional satellites. Various agencies and organizations have been developing novel solutions to this problem, before it turns into full-blown Kessler Syndrome. But many of them are reliant on understanding what is going on with the debris before attempting to deal with it. Gaining that understanding is hard, and failure to do so can cause satellites attempting to remove the debris to contribute to the problem rather than alleviating it. To help solve that conundrum, a new paper from researchers at GMV, a major player in the orbital tracking market in Europe, showcases a new algorithm that can use ground-based telescopes to try figure out how the debris is moving before a deorbiter gets anywhere near it.
The Primordial Black Hole Saga: Part 4 - Hidden Singularities
The challenge is that nothing in this universe is simple. And if there’s one thing you take away from today’s episode, then let it be that. Don’t ever let yourself fall into the trap of simple answers for difficult questions. We’re cosmologists, we study the universe as it is, not as we wish it would be.