Join the Alien Search, login or register FREE on Aliens and Space Forum

Members Can Post Anonymously On This Site

NASA’s Webb Discovers New Feature in Jupiter’s Atmosphere

By NASA
October 19, 2023 in NASA

https://www.aliensandspace.com/topic/10574-nasa%E2%80%99s-webb-discovers-new-feature-in-jupiter%E2%80%99s-atmosphere/

Image: Webb’s View of Jupiter

Jupiter dominates the black background of space. The image is a composite, and shows Jupiter in enhanced color, featuring the planet’s famous Great Red Spot, which appears white with light pink around the edges. The planet is striated with swirling horizontal stripes of green, periwinkle, light pink, and cream. Horizontally across the equator is a wide cream-colored band, whose height extends about 1/7 of the planet. This is the planet’s equatorial zone. The stripes across the planet interact and mix at their edges. Along both of the northern and southern poles, the planet glows in green. Bright red auroras glow just above the planet’s surface at both poles.

This image of Jupiter from NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) shows stunning details of the majestic planet in infrared light. In this image, brightness indicates high altitude. The numerous bright white ‘spots’ and ‘streaks’ are likely very high-altitude cloud tops of condensed convective storms. Auroras, appearing in red in this image, extend to higher altitudes above both the northern and southern poles of the planet. By contrast, dark ribbons north of the equatorial region have little cloud cover.

Image: NASA, ESA, CSA, STScI, R. Hueso (University of the Basque Country), I. de Pater (University of California, Berkeley), T. Fouchet (Observatory of Paris), L. Fletcher (University of Leicester), M. Wong (University of California, Berkeley), J. DePasquale (STScI)

“This is something that totally surprised us,” said Ricardo Hueso of the University of the Basque Country in Bilbao, Spain, lead author on the paper describing the findings. “What we have always seen as blurred hazes in Jupiter’s atmosphere now appear as crisp features that we can track along with the planet’s fast rotation.”

The research team analyzed data from Webb’s NIRCam (Near-Infrared Camera) captured in July 2022. The Early Release Science program – jointly led by Imke de Pater from the University of California, Berkeley and Thierry Fouchet from the Observatory of Paris – was designed to take images of Jupiter 10 hours apart, or one Jupiter day, in four different filters, each uniquely able to detect changes in small features at different altitudes of Jupiter’s atmosphere.

“Even though various ground-based telescopes, spacecraft like NASA’s Juno and Cassini, and NASA’s Hubble Space Telescope have observed the Jovian system’s changing weather patterns, Webb has already provided new findings on Jupiter’s rings, satellites, and its atmosphere,” de Pater noted.

While Jupiter is different from Earth in many ways – Jupiter is a gas giant, Earth is a rocky, temperate world – both planets have layered atmospheres. Infrared, visible, radio, and ultraviolet light wavelengths observed by these other missions detect the lower, deeper layers of the planet’s atmosphere – where gigantic storms and ammonia ice clouds reside.

Image: Jupiter’s Equatorial Jet Stream

The infographic shows Webb’s image of Jupiter at the left. The planet is striated with swirling horizontal stripes of neon turquoise, periwinkle, and cream. Below the planet, the NIRCam filters and their respective colors assigned are listed – F164N in blue, F212N in green, and F360M in red. On the right side of the infographic, there are 8 separate images. Two of those images are horizontal and span the entire right half of the infographic. The top horizontal image is labeled F212N 10:52 UT and the bottom is labeled F212N 20:55 UT. They are zoomed-in pullouts from a section of Jupiter’s equator—outlined in a white box on the image of the planet on the left. Both of these images are white and grey with horizontal wispy clouds. There are 6 smaller boxes in between the two horizontal images—3 rows of 2. The first column of the boxes is outlined in orange, the second column purple and the third yellow. Each of the smaller images correspond to orange, purple, and yellow boxes placed along the horizontal images.

On the other hand, Webb’s look farther into the near-infrared than before is sensitive to the higher-altitude layers of the atmosphere, around 15-30 miles (25-50 kilometers) above Jupiter’s cloud tops. In near-infrared imaging, high-altitude hazes typically appear blurry, with enhanced brightness over the equatorial region. With Webb, finer details are resolved within the bright hazy band.

The newly discovered jet stream travels at about 320 miles per hour (515 kilometers per hour), twice the sustained winds of a Category 5 hurricane here on Earth. It is located around 25 miles (40 kilometers) above the clouds, in Jupiter’s lower stratosphere.

By comparing the winds observed by Webb at high altitudes, to the winds observed at deeper layers from Hubble, the team could measure how fast the winds change with altitude and generate wind shears.

Image: Jupiter’s Winds

A portion of the graphic that displays wind speeds on Jupiter at different altitudes. The portion of this graphic shows the ends of three arrows that travel across the graphic from the left to the right. The top most arrow (colored in sky blue) extends the farthest right to about 3/4 the way across the graphic, the middle arrow (colored in periwinkle) extends to a little less than halfway across the graphic, and the bottom arrow (colored in light grey) extends to about 1/4 the way across the graphic. Extending out below each arrow is a cone of the same color to indicate the +/- error margin. There is Webb's image of Jupiter in the background of the graphic.

Researchers using NASA’s James Webb Space Telescope’s NIRCam (Near-Infrared Camera) have discovered a high-speed jet stream sitting over Jupiter’s equator, above the main cloud decks. At a wavelength of 2.12 microns, which observes between altitudes of about 12-21 miles (20-35 kilometers) above Jupiter’s cloud tops, researchers spotted several wind shears, or areas where wind speeds change with height or with distance, which enabled them to track the jet. This image highlights several of the features around Jupiter’s equatorial zone that, between one rotation of the planet (10 hours), are very clearly disturbed by the motion of the jet stream.

: NASA, ESA, CSA, STScI, Image: NASA, ESA, CSA, STScI, R. Hueso (University of the Basque Country), I. de Pater (University of California, Berkeley), T. Fouchet (Observatory of Paris), L. Fletcher (University of Leicester), M. Wong (University of California, Berkeley), A. James (STScI)

While Webb’s exquisite resolution and wavelength coverage allowed for the detection of small cloud features used to track the jet, the complementary observations from Hubble taken one day after the Webb observations were also crucial to determine the base state of Jupiter’s equatorial atmosphere and observe the development of convective storms in Jupiter’s equator not connected to the jet.

“We knew the different wavelengths of Webb and Hubble would reveal the three-dimensional structure of storm clouds, but we were also able to use the timing of the data to see how rapidly storms develop,” added team member Michael Wong of the University of California, Berkeley, who led the associated Hubble observations.

The researchers are looking forward to additional observations of Jupiter with Webb to determine if the jet’s speed and altitude change over time.

Image: Zoom in on Webb’s View of Jupiter

A zoomed in view of Webb’s Jupiter image.

“Jupiter has a complicated but repeatable pattern of winds and temperatures in its equatorial stratosphere, high above the winds in the clouds and hazes measured at these wavelengths,” explained team member Leigh Fletcher of the University of Leicester in the United Kingdom. “If the strength of this new jet is connected to this oscillating stratospheric pattern, we might expect the jet to vary considerably over the next 2 to 4 years – it’ll be really exciting to test this theory in the years to come.”

“It’s amazing to me that, after years of tracking Jupiter’s clouds and winds from numerous observatories, we still have more to learn about Jupiter, and features like this jet can remain hidden from view until these new NIRCam images were taken in 2022,” continued Fletcher.

The researchers’ results were recently published in Nature Astronomy.

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 the Canadian Space Agency.

Media Contacts

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

Hannah Braun – hbraun@stsci.edu , Christine Pulliam – cpulliam@stsci.edi
Space Telescope Science Institute, Baltimore, Md.

Downloads

Download full resolution images for this article from the Space Telescope Science Institute.

Related Information

NASA’s Jupiter Website – https://science.nasa.gov/jupiter/

NASA’s Solar System Website – https://science.nasa.gov/solar-system/

More Webb News – https://science.nasa.gov/mission/webb/latestnews/

More Webb Images – https://science.nasa.gov/mission/webb/multimedia/images/

Webb Mission Page – https://science.nasa.gov/mission/webb/

Keep Exploring

Details

Last Updated

Oct 19, 2023

Editor

Steve Sabia

Contact

Location

Goddard Space Flight Center

Related Terms

View the full article

Quote

Join the conversation

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

Reply to this topic...

× Pasted as rich text. Paste as plain text instead

Only 75 emoji are allowed.

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

× Your previous content has been restored. Clear editor

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

Insert image from URL

https://www.aliensandspace.com/topic/10574-nasa%E2%80%99s-webb-discovers-new-feature-in-jupiter%E2%80%99s-atmosphere/

Followers 0

Go to topic listing

Similar Topics
- NASA, International Astronauts Address Students from New York, Ohio
  By NASA
  
  Astronaut Anne McClain is pictured on May 1, 2025, near one of the International Space Station’s main solar arrays.Credit: NASA NASA astronaut Nichole Ayers and JAXA (Japan Aerospace Exploration Agency) astronaut Takuya Onishi will answer prerecorded questions submitted by middle and high school students from New York and Ohio. Both groups will hear from the astronauts aboard the International Space Station in two separate events.
  The first event at 10:20 a.m. EDT on Tuesday, May 20, includes students from Long Beach Middle School in Lido Beach, New York. Media interested in covering the event at Long Beach Middle School must RSVP no later than 5 p.m. Monday, May 19, to Christi Tursi at: ctursi@lbeach.org or 516-771-3960.
  The second event at 11 a.m. EDT on Friday, May 23, is with students from Vermilion High School in Vermilion, Ohio. Media interested in covering the event at Vermilion High School must RSVP no later than 5 p.m. Thursday, May 22, to Jennifer Bengele at: jbengele@vermilionschools.org or 440-479-7783.
  Watch both 20-minute Earth-to-space calls live on NASA STEM YouTube Channel.
  Long Beach Middle School will host the event for students in grades 6 through 8. The school aims to provide both the students and community with an experience that bridge gaps in space sciences with teaching and learning in classrooms.
  Vermilion High School will host the event for students in grades 9 through 12, to help increase student interest in science, technology, engineering, and mathematics career pathways.
  For more than 24 years, astronauts have continuously lived and worked aboard the space station, testing technologies, performing science, and developing skills needed to explore farther from Earth. Astronauts aboard the orbiting laboratory communicate with NASA’s Mission Control Center in Houston 24 hours a day through SCaN’s (Space Communications and Navigation) Near Space Network.
  Research and technology investigations taking place aboard the space station benefit people on Earth and lay the groundwork for other agency missions. As part of NASA’s Artemis campaign, the agency will send astronauts to the Moon to prepare for future human exploration of Mars, inspiring Artemis Generation explorers and ensuring the United States continues to lead in space exploration and discovery.
  See videos of astronauts aboard the space station at:
  https://www.nasa.gov/stemonstation
  -end-
  Gerelle Dodson
  Headquarters, Washington
  202-358-1600
  gerelle.q.dodson@nasa.gov
  Sandra Jones
  Johnson Space Center, Houston
  281-483-5111
  sandra.p.jones@nasa.gov
  Share
  Details
  Last Updated May 16, 2025 LocationNASA Headquarters Related Terms
  Humans in Space In-flight Education Downlinks International Space Station (ISS) Johnson Space Center Learning Resources NASA Headquarters View the full article
- Another First: NASA Webb Identifies Frozen Water in Young Star System
  By NASA
  
  Explore Webb Webb News Latest News Latest Images Webb’s Blog Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Observatory Overview Launch Deployment Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning 5 Min Read Another First: NASA Webb Identifies Frozen Water in Young Star System
  For the first time, researchers confirmed the presence of crystalline water ice in a dusty debris disk that orbits a Sun-like star, using NASA’s James Webb Space Telescope. The full artist’s concept illustration and full caption is shown below. Credits:
  NASA, ESA, CSA, Ralf Crawford (STScI) Is frozen water scattered in systems around other stars? Astronomers have long expected it is, partially based on previous detections of its gaseous form, water vapor, and its presence in our own solar system.
  Now there is definitive evidence: Researchers confirmed the presence of crystalline water ice in a dusty debris disk that orbits a Sun-like star 155 light-years away using detailed data known as spectra from NASA’s James Webb Space Telescope. (The term water ice specifies its makeup, since many other frozen molecules are also observed in space, such as carbon dioxide ice, or “dry ice.”) In 2008, data from NASA’s retired Spitzer Space Telescope hinted at the possibility of frozen water in this system.
  “Webb unambiguously detected not just water ice, but crystalline water ice, which is also found in locations like Saturn’s rings and icy bodies in our solar system’s Kuiper Belt,” said Chen Xie, the lead author of the new paper and an assistant research scientist at Johns Hopkins University in Baltimore, Maryland.
  All the frozen water Webb detected is paired with fine dust particles throughout the disk — like itsy-bitsy “dirty snowballs.” The results published Wednesday in the journal Nature.
  Astronomers have been waiting for this definitive data for decades. “When I was a graduate student 25 years ago, my advisor told me there should be ice in debris disks, but prior to Webb, we didn’t have instruments sensitive enough to make these observations,” said Christine Chen, a co-author and associate astronomer at the Space Telescope Science Institute in Baltimore. “What’s most striking is that this data looks similar to the telescope’s other recent observations of Kuiper Belt objects in our own solar system.”
  Water ice is a vital ingredient in disks around young stars — it heavily influences the formation of giant planets and may also be delivered by small bodies like comets and asteroids to fully formed rocky planets. Now that researchers have detected water ice with Webb, they have opened the door for all researchers to study how these processes play out in new ways in many other planetary systems.
  Image: Debris Disk Around Star HD 181327 (Artist’s Concept)
  For the first time, researchers confirmed the presence of crystalline water ice in a dusty debris disk that orbits a Sun-like star, using NASA’s James Webb Space Telescope. All the frozen water detected by Webb is paired with fine dust particles throughout the disk. The majority of the water ice observed is found where it’s coldest and farthest from the star. The closer to the star the researchers looked, the less water ice they found. NASA, ESA, CSA, Ralf Crawford (STScI) Rocks, Dust, Ice Rushing Around
  The star, cataloged HD 181327, is significantly younger than our Sun. It’s estimated to be 23 million years old, compared to the Sun’s more mature 4.6 billion years. The star is slightly more massive than the Sun, and it’s hotter, which led to the formation of a slightly larger system around it.
  Webb’s observations confirm a significant gap between the star and its debris disk — a wide area that is free of dust. Farther out, its debris disk is similar to our solar system’s Kuiper Belt, where dwarf planets, comets, and other bits of ice and rock are found (and sometimes collide with one another). Billions of years ago, our Kuiper Belt was likely similar to this star’s debris disk.
  “HD 181327 is a very active system,” Chen said. “There are regular, ongoing collisions in its debris disk. When those icy bodies collide, they release tiny particles of dusty water ice that are perfectly sized for Webb to detect.”
  Frozen Water — Almost Everywhere
  Water ice isn’t spread evenly throughout this system. The majority is found where it’s coldest and farthest from the star. “The outer area of the debris disk consists of over 20% water ice,” Xie said.
  The closer in the researchers looked, the less water ice they found. Toward the middle of the debris disk, Webb detected about 8% water ice. Here, it’s likely that frozen water particles are produced slightly faster than they are destroyed. In the area of the debris disk closest to the star, Webb detected almost none. It’s likely that the star’s ultraviolet light vaporizes the closest specks of water ice. It’s also possible that rocks known as planetesimals have “locked up” frozen water in their interiors, which Webb can’t detect.
  This team and many more researchers will continue to search for — and study — water ice in debris disks and actively forming planetary systems throughout our Milky Way galaxy. “The presence of water ice helps facilitate planet formation,” Xie said. “Icy materials may also ultimately be ‘delivered’ to terrestrial planets that may form over a couple hundred million years in systems like this.”
  The researchers observed HD 181327 with Webb’s NIRSpec (Near-Infrared Spectrograph), which is super-sensitive to extremely faint dust particles that can only be detected from space.
  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
  Downloads
  Click any image to open a larger version.
  View/Download all image products at all resolutions for this article from the Space Telescope Science Institute.
  View/Download the research results from the journal Nature.
  Media Contacts
  Laura Betz – laura.e.betz@nasa.gov
  NASA’s Goddard Space Flight Center, Greenbelt, Md.
  Claire Blome – cblome@stsci.edu
  Space Telescope Science Institute, Baltimore, Md.
  Christine Pulliam – cpulliam@stsci.edu
  Space Telescope Science Institute, Baltimore, Md.
  Related Information
  View Webb images of other debris disks around Vega, Fomalhaut, Beta Pictoris, and AU Microscopii
  Learn more about spectroscopy
  Read more: Webb’s Near-infrared Spectrograph (NIRSpec)
  More Webb News
  More Webb Images
  Webb Science Themes
  Webb Mission Page
  Related For Kids
  What is the Webb Telescope?
  SpacePlace for Kids
  En Español
  Ciencia de la NASA
  NASA en español
  Space Place para niños
  Keep Exploring Related Topics
  James Webb Space Telescope
  
  Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
  
  Stars
  
  Stars Stories
  
  Universe
  
  Share
  
  Details
  Last Updated May 14, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms
  James Webb Space Telescope (JWST) Astrophysics Goddard Space Flight Center Science & Research Stars The Universe View the full article
- Webb’s Titan Forecast: Partly Cloudy With Occasional Methane Showers
  By NASA
  
  Explore Webb Webb News Latest News Latest Images Webb’s Blog Awards X (offsite – login reqd) Instagram (offsite – login reqd) Facebook (offsite- login reqd) Youtube (offsite) Overview About Who is James Webb? Fact Sheet Impacts+Benefits FAQ Science Overview and Goals Early Universe Galaxies Over Time Star Lifecycle Other Worlds Observatory Overview Launch Deployment Orbit Mirrors Sunshield Instrument: NIRCam Instrument: MIRI Instrument: NIRSpec Instrument: FGS/NIRISS Optical Telescope Element Backplane Spacecraft Bus Instrument Module Multimedia About Webb Images Images Videos What is Webb Observing? 3d Webb in 3d Solar System Podcasts Webb Image Sonifications Team International Team People Of Webb More For the Media For Scientists For Educators For Fun/Learning 7 Min Read Webb’s Titan Forecast: Partly Cloudy With Occasional Methane Showers
  These images of Titan were taken by NASA’s James Webb Space Telescope on July 11, 2023 (top row) and the ground-based W.M. Keck Observatories on July 14, 2023 (bottom row). They show methane clouds appearing at different altitudes in Titan’s northern hemisphere. Full image and description below. Credits:
  NASA, ESA, CSA, STScI, and W.M. Keck Observatories Saturn’s moon Titan is an intriguing world cloaked in a yellowish, smoggy haze. Similar to Earth, the atmosphere is mostly nitrogen and has weather, including clouds and rain. Unlike Earth, whose weather is driven by evaporating and condensing water, frigid Titan has a methane cycle.
  NASA’s James Webb Space Telescope, supplemented with images from the Keck II telescope, has for the first time found evidence for cloud convection in Titan’s northern hemisphere, over a region of lakes and seas. Webb also has detected a key carbon-containing molecule that gives insight into the chemical processes in Titan’s complex atmosphere.
  Titan’s Weather
  On Titan, methane plays a similar role to water on Earth when it comes to weather. It evaporates from the surface and rises into the atmosphere, where it condenses to form methane clouds. Occasionally it falls as a chilly, oily rain onto a solid surface where water ice is hard as rocks.
  “Titan is the only other place in our solar system that has weather like Earth, in the sense that it has clouds and rainfall onto a surface,” explained lead author Conor Nixon of NASA’s Goddard Space Flight Center in Greenbelt, Maryland.
  The team observed Titan in November 2022 and July 2023 using both Webb and one of the twin ground-based W.M. Keck Observatories telescopes. Those observations not only showed clouds in the mid and high northern latitudes on Titan – the hemisphere where it is currently summer – but also showed those clouds apparently rising to higher altitudes over time. While previous studies have observed cloud convection at southern latitudes, this is the first time evidence for such convection has been seen in the north. This is significant because most of Titan’s lakes and seas are located in its northern hemisphere and evaporation from lakes is a major potential methane source. Their total area is similar to that of the Great Lakes in North America.
  On Earth the lowest layer of the atmosphere, or troposphere, extends up to an altitude of about 7 miles (12 kilometers). However, on Titan, whose lower gravity allows the atmospheric layers to expand, the troposphere extends up to about 27 miles (45 kilometers). Webb and Keck used different infrared filters to probe to different depths in Titan’s atmosphere, allowing astronomers to estimate the altitudes of the clouds. The science team observed clouds that appeared to move to higher altitudes over a period of days, although they were not able to directly see any precipitation occurring.
  Image A: Titan (Webb and Keck Image)
  These images of Titan were taken by NASA’s James Webb Space Telescope on July 11, 2023 (top row) and the ground-based W.M. Keck Observatories on July 14, 2023 (bottom row). They show methane clouds (denoted by the white arrows) appearing at different altitudes in Titan’s northern hemisphere. On the left side are representative-color images from both telescopes. In the Webb image light at 1.4 microns is colored blue, 1.5 microns is green, and 2.0 microns is red (filters F140M, F150W, and F200W, respectively). In the Keck image light at 2.13 microns is colored blue, 2.12 microns is green, and 2.06 microns is red (H2 1-0, Kp, and He1b, respectively).
  In the middle column are single-wavelength images taken by Webb and Keck at 2.12 microns. This wavelength is sensitive to emission from Titan’s lower troposphere. The rightmost images show emission at 1.64 microns (Webb) and 2.17 microns (Keck), which favor higher altitudes, in Titan’s upper troposphere and stratosphere (an atmospheric layer above the troposphere). It demonstrates that the clouds are seen at higher altitudes on July 14 than earlier on July 11, indicative of upward motion.
  
  NASA, ESA, CSA, STScI, and W.M. Keck Observatories Titan’s Chemistry
  Titan is an object of high astrobiological interest due to its complex organic (carbon-containing) chemistry. Organic molecules form the basis of all life on Earth, and studying them on a world like Titan may help scientists understand the processes that led to the origin of life on Earth.
  The basic ingredient that drives much of Titan’s chemistry is methane, or CH4. Methane in Titan’s atmosphere gets split apart by sunlight or energetic electrons from Saturn’s magnetosphere, and then recombines with other molecules to make substances like ethane (C2H6) along with more complex carbon-bearing molecules.
  Webb’s data provided a key missing piece for our understanding of the chemical processes: a definitive detection of the methyl radical CH3. This molecule (called “radical” because it has a “free” electron that is not in a chemical bond) forms when methane is broken apart. Detecting this substance means that scientists can see chemistry in action on Titan for the first time, rather than just the starting ingredients and the end products.
  “For the first time we can see the chemical cake while it’s rising in the oven, instead of just the starting ingredients of flour and sugar, and then the final, iced cake,” said co-author Stefanie Milam of the Goddard Space Flight Center.
  Image B: Chemistry in Titan’s Atmosphere
  This four-panel infographic demonstrates a key chemical process believed to occur in the atmosphere of Saturn’s moon Titan.
  1. Titan has a thick, nitrogen (N2) atmosphere that also contains methane (CH4).
  2. Molecules known as methyl radicals (CH3) form when methane is broken apart by sunlight or energetic electrons from Saturn’s magnetosphere.
  3. It then recombines with other molecules or with itself to make substances like ethane (C2H6).
  4. Methane, ethane, and other molecules condense and rain out of the atmosphere, forming lakes and seas on Titan’s surface. NASA’s James Webb Space Telescope detected the methyl radical on Titan for the first time, providing a key missing piece for our understanding of Titan’s chemical processes.
  NASA, ESA, CSA, and Elizabeth Wheatley (STScI) The Future of Titan’s Atmosphere
  This hydrocarbon chemistry has long-term implications for the future of Titan. When methane is broken apart in the upper atmosphere, some of it recombines to make other molecules that eventually end up on Titan’s surface in one chemical form or another, while some hydrogen escapes from the atmosphere. As a result, methane will be depleted over time, unless there is some source to replenish it.
  A similar process occurred on Mars, where water molecules were broken up and the resulting hydrogen lost to space. The result was the dry, desert planet we see today.
  “On Titan, methane is a consumable. It’s possible that it is being constantly resupplied and fizzing out of the crust and interior over billions of years. If not, eventually it will all be gone and Titan will become a mostly airless world of dust and dunes,” said Nixon.
  Video: Webb Spies Rain Clouds, New Molecule on Titan
  Of all the alien worlds in our solar system, one in particular resembles our home planet. Titan, the largest moon of Saturn, is the only other place we know of where you could walk along the seashore or stand in the rain. However, Titan’s exotic seas and its oily raindrops are not made of water, but of the natural gases methane and ethane, super-chilled into liquid form. Now, NASA’s James Webb Space Telescope has revealed a crucial, missing step in how ethane is formed, and its discovery could tell us about the future of Titan’s atmosphere. Credit: NASA’s Goddard Space Flight Center. Producer/Editor: Dan Gallagher. Lead Scientist/Narrator: Conor Nixon. Lead Animator: Jenny McElligott. Lead Visualizer: Andrew J Christensen. Scientist: Nicholas Lombardo. Animator/Art Director: Michael Lentz. Animation Lead: Walt Feimer. Animators: Jonathan North, Wes Buchanan, Kim Dongjae, Chris Meaney, Adriana Manrique Gutierrez. Data Visualizers: Mark SubbaRao, Kel Elkins, Ernie Wright. Data Provider: Juan Lora. Executive Producer: Wade Sisler. Social Media Support: Kathryn Mersmann. Public Affairs: Laura Betz.
  Complementing the Dragonfly Mission
  More of Titan’s mysteries will be probed by NASA’s Dragonfly mission, a robotic rotorcraft scheduled to land on Saturn’s moon in 2034. Making multiple flights, Dragonfly will explore a variety of locations. Its in-depth investigations will complement Webb’s global perspective.
  “By combining all of these resources, including Webb, NASA’s Hubble Space Telescope, and ground-based observatories, we maintain continuity between the former Cassini/Huygens mission to Saturn and the upcoming Dragonfly mission,” added Heidi Hammel, vice president of the Association of Universities for Research in Astronomy and a Webb Interdisciplinary Scientist.
  This data was taken as part of Hammel’s Guaranteed Time Observations program to study the Solar System. The results were published in the journal Nature Astronomy.
  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
  Downloads
  Click any image to open a larger version.
  View/Download all image products at all resolutions for this article from the Space Telescope Science Institute.
  View/Download the research results from the journal Nature Astronomy.
  Media Contacts
  Laura Betz – laura.e.betz@nasa.gov
  NASA’s Goddard Space Flight Center, Greenbelt, Md.
  Christine Pulliam – cpulliam@stsci.edu
  Space Telescope Science Institute, Baltimore, Md.
  Science
  Conor Nixon (NASA-GSFC), Heidi Hammel (AURA)
  Related Information
  Learn more about Titan
  Read more: Webb’s Near-infrared Spectrograph (NIRSpec)
  Webb Blog: Webb, Keck Telescopes Team Up to Track Clouds on Saturn’s Moon Titan
  More Webb News
  More Webb Images
  Webb Science Themes
  Webb Mission Page
  Related For Kids
  What is the Webb Telescope?
  SpacePlace for Kids
  En Español
  Ciencia de la NASA
  NASA en español
  Space Place para niños
  Keep Exploring Related Topics
  James Webb Space Telescope
  
  Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
  
  Titan
  
  Saturn and Titan Resources
  
  This page showcases our resources for those interested in learning more about Saturn and Titan.
  
  Dragonfly
  
  Share
  
  Details
  Last Updated May 14, 2025 Editor Marty McCoy Contact Laura Betz laura.e.betz@nasa.gov Related Terms
  James Webb Space Telescope (JWST) Astrophysics Goddard Space Flight Center Planets Saturn Saturn Moons Science & Research The Solar System Titan View the full article
- Take a Tour of the Cosmos with New Interactives from NASA’s Universe of Learning
  By NASA
  
  Explore This Section Science Science Activation Take a Tour of the Cosmos with… Overview Learning Resources Science Activation Teams SME Map Opportunities More Science Activation Stories Citizen Science 4 min read
  Take a Tour of the Cosmos with New Interactives from NASA’s Universe of Learning
  Ready for a tour of the cosmos? NASA’s Universe of Learning has released a new, dynamic way for lifelong learners to explore NASA’s breathtaking images of the universe—ViewSpace interactive Image Tours. ViewSpace has an established track record of providing museums, science centers, libraries, and other informal learning environments with free, web-based videos and digital interactives—like its interactive Image Sliders. These new Image Tours are another unique experience from NASA’s Universe of Learning, created through a collaboration between scientists that operate NASA telescopes and experts well-versed in the most modern methods of learning. Hands-on, self-directed learning resources like these have long been valued by informal learning sites as effective means for engaging and intriguing users with the latest discoveries from NASA’s space telescope missions—while encouraging lifelong learners to continue their passionate exploration of the stars, galaxies, and distant worlds.
  With these new ViewSpace Image Tours, visitors can take breathtaking journeys through space images that contain many exciting stories. The “Center of the Milky Way Galaxy” Tour, for example, uses breathtaking images from NASA’s Hubble, Spitzer, and Chandra X-ray telescopes and includes eleven Tour Stops, where users can interact with areas like “the Brick”—a dense, dark cloud of hydrogen molecules imaged by Spitzer. Another Tour Stop zooms toward the supermassive black hole, Sagittarius A*, offering a dramatic visual journey to the galaxy’s core.
  In other tours, like the “Herbig-Haro 46/47” Tour, learners can navigate through points of interest in an observation from a single telescope mission. In this case, NASA’s James Webb Space Telescope provides the backdrop where lifelong learners can explore superheated jets of gas and dust being ejected at tremendous speeds from a pair of young, forming stars. The power of Webb turns up unexpected details in the background, like a noteworthy distant galaxy famous for its uncanny resemblance to a question mark. Each Interactive Image Tour allows people to examine unique features through videos, images, or graphical overlays to identify how those features have formed in ways that static images alone can’t convey.
  These tours, which include detailed visual descriptions for each Tour Stop, illuminate the science behind the beauty, allowing learners of all ages to develop a greater understanding of and excitement for space science, deepening their engagement with astronomy, regardless of their prior experience. Check out the About the Interactives page on the ViewSpace website for a detailed overview of how to use the Image Tours.
  ViewSpace currently offers three Image Tours, and the collection will continue growing:
  Center of the Milky Way Galaxy:
  Peer through cosmic dust and uncover areas of intense activity near the Milky Way’s core, featuring imagery from the Hubble Space Telescope, Spitzer Space Telescope, and the Chandra X-ray Observatory.
  Herbig-Haro 46/47:
  Witness how a tightly bound pair of young stars shapes their nebula through ejections of gas and dust in an image from the James Webb Space Telescope.
  The Whirlpool Galaxy:
  Explore the iconic swirling arms and glowing core of a stunning spiral galaxy, with insights into star formation, galaxy structure, and more in a Hubble Space Telescope image.
  “The Image Tours are beautiful, dramatic, informational, and easy to use,” explained Sari Custer, Chief of Science and Curiosity at Arizona Science Center. “I’m excited to implement them in my museum not only because of the incredible images and user-friendly features, but also for the opportunity to excite and ignite the public’s curiosity about space.”
  NASA’s Universe of Learning is supported by NASA under cooperative agreement award number NNX16AC65A and is part of NASA’s Science Activation Portfolio. Learn more about how Science Activation connects NASA science experts, real content, and experiences with community leaders to do science in ways that activate minds and promote deeper understanding of our world and beyond: https://science.nasa.gov/learn/about-science-activation/
  Select views from various Image Tours. Clockwise from top left: The Whirlpool Galaxy, Center of the Milky Way Galaxy, Herbig-Haro 46/47, detail view in the Center of the Milky Way Galaxy. Share
  
  Details
  Last Updated May 13, 2025 Editor NASA Science Editorial Team Related Terms
  Science Activation Astrophysics For Educators Explore More
  5 min read NASA’s Webb Reveals New Details, Mysteries in Jupiter’s Aurora
  
  Article
  
  1 day ago
  2 min read Hubble Comes Face-to-Face with Spiral’s Arms
  
  Article
  
  4 days ago
  7 min read NASA’s Hubble Pinpoints Roaming Massive Black Hole
  
  Article
  
  5 days ago
  Keep Exploring Discover More Topics From NASA
  James Webb Space Telescope
  
  Webb is the premier observatory of the next decade, serving thousands of astronomers worldwide. It studies every phase in the…
  
  Perseverance Rover
  
  This rover and its aerial sidekick were assigned to study the geology of Mars and seek signs of ancient microbial…
  
  Parker Solar Probe
  
  On a mission to “touch the Sun,” NASA’s Parker Solar Probe became the first spacecraft to fly through the corona…
  
  Juno
  
  NASA’s Juno spacecraft entered orbit around Jupiter in 2016, the first explorer to peer below the planet’s dense clouds to…
  
  View the full article
- Jupiter’s Turbulent Atmosphere
  By NASA
  
  Image data: NASA/JPL-Caltech/SwRI/MSSS; Image processing: Jackie Branc (CC BY) JunoCam, the visible light imager aboard NASA’s Juno spacecraft, captured this view of Jupiter’s northern high latitudes during the spacecraft’s 69th flyby of the giant planet on Jan. 28, 2025. Jupiter’s belts and zones stand out in this enhanced color rendition, along with the turbulence along their edges caused by winds going in different directions.
  The original JunoCam data used to produce this view was taken from an altitude of about 36,000 miles (58,000 kilometers) above Jupiter’s cloud tops. JunoCam’s raw images are available for the public to peruse and process into image products. Citizen scientist Jackie Branc processed the image.
  Since Juno arrived at Jupiter in 2016, it has been probing beneath the dense, forbidding clouds encircling the giant planet – the first orbiter to peer so closely. It seeks answers to questions about the origin and evolution of Jupiter, our solar system, and giant planets across the cosmos.
  Learn more about NASA citizen science.
  Image credit: Image data: NASA/JPL-Caltech/SwRI/MSSS; Image processing: Jackie Branc (CC BY)
  View the full article
Check out these Videos

Sign In

NASA’s Webb Discovers New Feature in Jupiter’s Atmosphere

Recommended Posts

NASA

Image: Webb’s View of Jupiter

Image: Jupiter’s Equatorial Jet Stream

Image: Jupiter’s Winds

Image: Zoom in on Webb’s View of Jupiter

Media Contacts

Downloads

Related Information

Related Topics

Jupiter

Our Solar System

Planets

Universe

Share

Details

Related Terms

Join the conversation

Similar Topics

Check out these Videos

Activity

Browse

Videos