Skip to main content

Saturn as you’ve never seen it before, captured by Webb telescope

Saturn captured by the James Webb Space Telescope
NASA, ESA, CSA, JWST Saturn team

NASA has shared a gorgeous image of Saturn captured recently by the James Webb Space Telescope (JWST).

Webb’s first near-infrared observations of the second largest planet in our solar system also show several of Saturn’s moons: Dione, Enceladus, and Tethys.

Saturn and three of its moons, captured by the James Webb Space Telescope
Saturn and three of its moons, captured by the James Webb Space Telescope NASA, ESA, CSA, JWST Saturn team

In the image, Saturn itself appears darker than you might expect, but that’s because of the infrared wavelength being used to observe the celestial body, as methane gas absorbs almost all of the sunlight falling on the atmosphere.

Saturn’s icy rings, on the other hand, lack methane and so really stand out, giving us an unusual view of the sixth planet from the sun.

Webb turned its attention to Saturn as part of an exercise to test the space telescope’s potential for detecting faint moons around the planet and its bright rings.

“Any newly discovered moons could help scientists put together a more complete picture of the current system of Saturn, as well as its past,” NASA said.

The early results are promising, with plenty of detail captured within Saturn’s ring system.

NASA said that even deeper exposures will enable researchers to better analyze some of Saturn’s fainter rings, which comprise rocky and icy fragments that range in size “from smaller than a grain of sand to a few as large as mountains on Earth.”

Over the past few decades, Saturn has been observed by other missions such as NASA’s Pioneer 11, Voyager 1 and Voyager 2, the Cassini spacecraft, and the Hubble Space Telescope. But using its near-infrared camera, the powerful Webb telescope, which started sending back stunning images of deep space last year, offers researchers an excellent chance to deepen their understanding of the planet and perhaps discover new features and characteristics over the coming years.

“We are very pleased to see JWST produce this beautiful image, which is confirmation that our deeper scientific data also turned out well,” Dr. Matthew Tiscareno, a senior research scientist at the SETI Institute who led the process of designing this observation, said in a statement. “We look forward to digging into the deep exposures to see what discoveries may await.”

Did you know you can even see Saturn with the naked eye? These excellent astronomy apps show you how.

Editors' Recommendations

Trevor Mogg
Contributing Editor
Not so many moons ago, Trevor moved from one tea-loving island nation that drives on the left (Britain) to another (Japan)…
James Webb telescope captures a dramatic image of newborn star
The NASA/ESA/CSA James Webb Space Telescope reveals intricate details of the Herbig Haro object 797 (HH 797). Herbig-Haro objects are luminous regions surrounding newborn stars (known as protostars), and are formed when stellar winds or jets of gas spewing from these newborn stars form shockwaves colliding with nearby gas and dust at high speeds. HH 797, which dominates the lower half of this image, is located close to the young open star cluster IC 348, which is located near the eastern edge of the Perseus dark cloud complex. The bright infrared objects in the upper portion of the image are thought to host two further protostars. This image was captured with Webb’s Near-InfraRed Camera (NIRCam).

A new image of a Herbig-Haro object captured by the James Webb Space Telescope shows the dramatic outflows from a young star. These luminous flares are created when stellar winds shoot off in opposite directions from newborn stars, as the jets of gas slam into nearby dust and gas at tremendous speed. These objects can be huge, up to several light-years across, and they glow brightly in the infrared wavelengths in which James Webb operates.

This image shows Herbig-Haro object HH 797, which is located close to the IC 348 star cluster, and is also nearby to another Herbig-Haro object that Webb captured recently: HH 211.

Read more
James Webb finds that rocky planets could form in extreme radiation environment
This is an artist’s impression of a young star surrounded by a protoplanetary disk in which planets are forming.

It takes a particular confluence of conditions for rocky planets like Earth to form, as not all stars in the universe are conducive to planet formation. Stars give off ultraviolet light, and the hotter the star burns, the more UV light it gives off. This radiation can be so significant that it prevents planets from forming from nearby dust and gas. However, the James Webb Space Telescope recently investigated a disk around a star that seems like it could be forming rocky planets, even though nearby massive stars are pumping out huge amounts of radiation.

The disk of material around the star, called a protoplanetary disk, is located in the Lobster Nebula, one of the most extreme environments in our galaxy. This region hosts massive stars that give off so much radiation that they can eat through a disk in as little as a million years, dispersing the material needed for planets to form. But the recently observed disk, named XUE 1, seems to be an exception.

Read more
How astronomers used James Webb to detect methane in the atmosphere of an exoplanet
An artists rendering of a blue and white exoplanet known as WASP-80 b, set on a star-studded black background. Alternating horizontal layers of cloudy white, grey and blue cover the planets surface. To the right of the planet, a rendering of the chemical methane is depicted with four hydrogen atoms bonded to a central carbon atom, representing methane within the exoplanet's atmosphere. An artist’s rendering of the warm exoplanet WASP-80 b whose color may appear bluish to human eyes due to the lack of high-altitude clouds and the presence of atmospheric methane identified by NASA’s James Webb Space Telescope, similar to the planets Uranus and Neptune in our own solar system.

One of the amazing abilities of the James Webb Space Telescope is not just detecting the presence of far-off planets, but also being able to peer into their atmospheres to see what they are composed of. With previous telescopes, this was extremely difficult to do because they lacked the powerful instruments needed for this kind of analysis, but scientists using Webb recently announced they had made a rare detection of methane in an exoplanet atmosphere.

Scientists studied the planet WASP-80 b using Webb's NIRCam instrument, which is best known as a camera but also has a slitless spectroscopy mode which allows it to split incoming light into different wavelengths. By looking at which wavelengths are missing because they have been absorbed by the target, researchers can tell what an object -- in this case, a planetary atmosphere -- is composed of.

Read more