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- The James Webb Space Telescope<\/strong> has discovered and directly imaged its first exoplanet. It\u2019s the first one Webb has found that other telescopes hadn\u2019t previously found.<\/li>\n
- The planet, TWA 7 b<\/strong> (labeled as CC #1 on the image above), has about the same mass as Saturn and is 111 light-years away. It\u2019s the least massive exoplanet imaged so far.<\/li>\n
- The discovery is a significant step<\/strong> toward astronomers being able to image even smaller and less massive exoplanets.<\/li>\n<\/ul>\n
Webb discovers its 1st exoplanet<\/h3>\n
NASA\u2019s James Webb Space Telescope has studied a growing number of exoplanets, or planets that orbit other stars. Now, it has discovered<\/em> its first exoplanet and directly imaged it. Researchers with the National Centre for Scientific Research (CNRS) in France \u2013 led by Anne-Marie Lagrange \u2013 said on June 25, 2025, that Webb found the planet in the circumstellar disk of a young star called TWA 7 (aka CE Antliae), about 111 light-years from Earth. This is the first time Webb has discovered a new exoplanet as opposed to observing previously discovered ones. This is also the least massive planet that astronomers have directly imaged so far.<\/p>\n
Webb used its Mid-Infared Instrument (MIRI) to find the planet.<\/p>\n
With a mass similar to Saturn, the new exoplanet \u2013 dubbed TWA 7 b \u2013 is 10 times less massive than any previously imaged exoplanet. The discovery is a significant step toward being able to image even less massive and smaller exoplanets in the future.<\/p>\n
The researchers published the peer-reviewed details of the discovery in Nature<\/em> on June 25, 2025.<\/p>\n
Young exoplanet is least massive imaged so far<\/h3>\n
Webb has observed many different exoplanets since it began its mission in 2022. But that focus has been on those previously discovered by other telescopes. Now the mighty Webb has snagged its own first exoplanet, TWA 7 b. The planet orbits the young red dwarf star TWA 7 (aka CE Antliae), which is about 111 light-years from Earth in the constellation Antlia. Astronomers first discovered the star in 1999.<\/p>\n
Since the star is only a few million years old, it still has a circumstellar disk of gas and dust surrounding it. It is in those disks that planets are born. The researchers looked for signs of possible planets forming in the disk of TWA 7, and they found one.<\/p>\n
The planet\u2019s mass is similar to that of Saturn, and it\u2019s 10 times less massive than any exoplanet previously detected in direct images. Of course, as it so far away, it still just looks like a bright dot, even in Webb images.<\/p>\n
![\"3](\"https:\/\/earthsky.org\/upl\/2025\/06\/TWA7b-Webb-February-20-2025.png\")
View larger. | Another view of the TWA 7 system from Webb. The bright spot labeled CC #1 is the planet. A background star and galaxy are also seen here. Image via A.-M. Lagrange and al.\/ arXiv.<\/figcaption><\/figure>\n Seeing the disk from above<\/h3>\n
As with some other circumstellar disks, this one is facing toward us, so Webb sees the full disk \u201cfrom above.\u201d Also, the disk around TWA 7 has three distinct concentric rings in it. Astronomers said that such rings form as a result of the gravitational influence of newly forming planets. The suspected planet also has a clear space around it within the ring that it resides in. This is consistent with a planet forming and sweeping up material in its vicinity. That, in turn, suggests this is truly a planet and not a background star or galaxy.<\/p>\n
The researchers used computer simulations to try to further determine if TWA 7 b was really a planet. These simulations helped confirm the thin ring in the circumstellar disk that the planet is in, as well as the \u201chole\u201d in the disk at the exact location of the suspected planet. This again supports TWA 7 b being a real planet.<\/p>\n
The planet is still young and forming as material from the circumstellar disk coalesces together. As a result, it appears brighter (hotter) in mid-infrared images than older planets do.<\/p>\n
![\"Black](\"https:\/\/earthsky.org\/upl\/2025\/06\/Anne-Marie-Lagrange-National-Center-for-Scientific-Research.jpg\")
Anne-Marie Lagrange, Research Director at the French National Center for Scientific Research (CNRS), led the new study about TWA 7 b. Image via CNRS.<\/figcaption><\/figure>\n The Hubble Space Telescope first imaged the circumstellar disk of TWA 7 in scattered light in 1998. Reprocessing of the data in 2016 helped to reveal the details of the disk itself.<\/p>\n
Imaging smaller and less massive planets<\/h3>\n
The discovery proves that Webb is well-suited for finding exoplanets. TWA 7 b has a mass approximately 30% that of Jupiter, or similar to Saturn. The researchers said Webb should be able to find and image planets only 10% the mass of Jupiter. That would be a big step toward imaging even smaller, rocky planets about the size of Earth. We already know they exist from detections made by other telescopes, but directly imaging them is still a challenge. The two most-used techniques are the transit method and radial velocity.<\/p>\n
Bottom line: NASA\u2019s James Webb Space Telescope has discovered its first exoplanet. TWA 7 b orbits a red dwarf star 111 light-years away and has a mass similar to Saturn.<\/p>\n
Source: Evidence for a sub-jovian planet in the young TWA7 disk<\/p>\n
Source (preprint): Evidence for a sub-jovian planet in the young TWA7 disk<\/p>\n
Via National Centre for Scientific Research<\/p>\n
<\/div>\n
\n - The planet, TWA 7 b<\/strong> (labeled as CC #1 on the image above), has about the same mass as Saturn and is 111 light-years away. It\u2019s the least massive exoplanet imaged so far.<\/li>\n