JWST Spots Signs of Exomoon Birth in Alien Planet’s DiskNEWS | 02 December 2025I agree my information will be processed in accordance with the Scientific American and Springer Nature Limited Privacy Policy . We leverage third party services to both verify and deliver email. By providing your email address, you also consent to having the email address shared with third parties for those purposes.
For the first time, scientists have directly detected molecules in a Frisbee of gas and dust swirling around an alien gas-giant planet. “I didn’t think this was possible,” says astronomer Sierra Grant of Carnegie Science in Washington, D.C. Typically such a faint signal would be invisible in the glare of a star. Grant and her co-author Gabriele Cugno of the University of Zürich, who published the results recently in the Astrophysical Journal Letters, think the carbon-rich disk is a lunar nursery and already have plans to observe several more; eventually researchers might be able to detect gaps carved in such disks by nascent moons.
Grant and Cugno used the James Webb Space Telescope (JWST) to pick out the infrared glow from the disk of gas and dust encircling a Goliath world called CT Cha b. Spotting light cast by a planet—let alone a disk around one—is like making out a firefly against a floodlight. It’s easier if the firefly is enormous and far away from the light. CT Cha b weighs a whopping 14 to 24 Jupiter masses and orbits its star about 17 times farther out than Neptune does the sun.
Previous observations had hinted that CT Cha b was gobbling up material from a yet unseen disk, and Cugno aimed to disentangle this disk’s glow of infrared heat from the star’s bright gleam. Grant was skeptical it could be done, but Cugno wanted to test JWST’s limits. “It was almost a game,” he says.
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Cugno ultimately pulled a “beautiful” light spectrum of the disk out of the data, in which Grant spotted clear chemical fingerprints of carbon-rich compounds such as hydrogen cyanide, acetylene and even molecules as complex as six-carbon benzene rings—substances absent from the material swirling directly around CT Cha b’s star. The disk could be a moon-building zone around the planet.
“This might give us a hint about what material is available for the formation of exomoons,” says astrophysicist Danny Gasman of the Max Planck Institute for Astronomy in Germany, who wasn’t involved in the study. She cautions, however, that although CT Cha b’s size and extreme distance from its star make it a great target, they also mean that it might be more like a failed star than a typical gas giant.
Even in our own solar system, the origins of moons remain mysterious. Disks such as CT Cha b’s offer a chance to understand not only moons of alien systems but also the moons in ours. “It’s really hard to go back in time 4.5 billion years and imagine how they were created,” Cugno says. “Now we can actually see this process.”Author: Sarah Lewin Frasier. Elise Cutts. Source
