JWST Made The First Detection Of Carbon-Rich Molecules In The Gas-Dust Disk Around CT Cha b (~620 Ly Away). The Disk May Form Exomoons Via A Hydrocarbon-Dominated Path Unlike Our Solar System Moons. CT Cha b Has 14–24 Jupiter Masses And Orbits Far From Its Star, Blurring If It’s A Planet Or A Failed Star, But Offers Clues To Moon Formation.
JWST Spots Signs of Exomoon Birth in Alien Planet’s DiskFor 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.




